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POST MEETING REPORT

1. Meeting Number: IAU Symposium 278

2. Meeting Title: Archaeoastronomy and Ethnoastronomy: Building Bridges between Cultures (Ninth “Oxford” International Symposium on Archaeoastronomy)

3. Co-ordinating Division: Division XII

4. Dedication of meeting None

5. Location , Peru

6. Dates of meeting: Jan 5–14, 2011

7. Number of participants: 120

8. List of represented Argentina, Australia, Austria, Bolivia, Brazil, Canada, Chile, Col- countries: ombia, Czech Republic, Egypt, Italy, Japan, Mexico, New Zealand, Nigeria, Peru, Poland, Spain, Switzerland, Thailand, UK, USA

9. Report submitted by: Clive Ruggles

10. Date and place: Leicester, Feb 7, 2011

11. Signature of SOC Chair:

ATTACHED DOCUMENTS

APPENDIX I — Final scientific programme APPENDIX II — List of participants APPENDIX III — List of recipients of IAU grants ***NB The receipts signed by the recipients of IAU Grants were sent by post on Feb 2, 2011 APPENDIX IV — Brief report to the Executive Committee

An on-line form has been submitted for "Women in " statistics. “OXFORD IX” IAU SYMPOSIUM 278

NINTH “OXFORD” INTERNATIONAL SYMPOSIUM ON ARCHAEOASTRONOMY NOVENO SIMPOSIO INTERNACIONAL “OXFORD” SOBRE ARQUEOASTRONOMÍA NONO SIMPÓSIO INTERNACIONAL “OXFORD” SOBRE ARQUEOASTRONOMIA

Archaeoastronomy and Ethnoastronomy: Building Bridges between Cultures

Arqueoastronomía y Etnoastronomía: Construyendo Puentes entre Culturas

Arqueoastronomia e Etnoastronomia: Construindo Pontes entre Culturas

LIMA, PERÚ, 2011

— 2 —

PROGRAMME PROGRAMA

Sunrise at Chankillo. © Ivan Ghezzi — 3 —

OVERALL SCHEDULE OF EVENTS

Tuesday, January 4

Time Event Venue* 14:00–18:00 Registration desk open CCPB

Wednesday, January 5

08:00–17:30 Registration desk open CCPB 09:00–10:45 MAIN CONFERENCE OPENING SESSION CCPB 10:45–11:30 Coffee and posters CCPB 11:30–13:00 MAIN CONFERENCE SESSION CCPB 13:00–15:00 Lunch 15:00–16:45 MAIN CONFERENCE SESSION CCPB 16:45–17:15 Coffee and posters CCPB 17:15–19:00 MAIN CONFERENCE SESSION CCPB 20:00– Welcoming reception at the CCPB (accompanying people welcome) CCPB

Thursday, January 6

08:30–17:30 Registration desk open CCPB 09:00–10:45 MAIN CONFERENCE SESSION CCPB 10:45–11:15 Coffee and posters CCPB 11:30–13:00 MAIN CONFERENCE SESSION CCPB 13:00–15:00 Lunch 15:00–16:45 MAIN CONFERENCE SESSION CCPB 16:45–17:15 Coffee and posters CCPB 17:15–19:00 MAIN CONFERENCE SESSION CCPB 20:00 Welcoming reception at the PUCP (accompanying people welcome) CCPU 21:00 Public lecture by Gary Urton (see page 9) CCPU

*Venues: CCPB Centro Cultural Peruano Británico, Bellavista 531, Miraflores CAPC Casa Andina Private Collection hotel, Av. La Paz 463, Miraflores. See conference website for map CCPU: Centro Cultural of the Pontificia Universidad Católica del Perú, Av. Camino Real 1075, San Isidro PUCP : Main campus of the PUCP, Av. Universitaria 1801, San Miguel. Building H, Rooms 103/104/205 RHP: Restaurant Huaca Pucllana, General Borgoño Cdra. 8, Miraflores — 4 —

Friday, January 7

Time Event Venue* 08:30–11:00 Registration desk open CCPB 09:00–10:30 MAIN CONFERENCE SESSION CCPB 10:30–11:00 Coffee CCPB 11:00–19:00 Excurssion to Puruchuco 20:00– Folklore event CCPB

Saturday, January 8

08:30–17:30 Registration desk open CCPB 09:00–10:30 MAIN CONFERENCE SESSION CCPB 10:30–11:00 Coffee and posters CCPB 11:00–13:00 MAIN CONFERENCE SESSION CCPB 13:00–15:00 Lunch 15:00–16:30 MAIN CONFERENCE SESSION CCPB 16:30–17:00 Coffee and posters CCPB 17:00–19:00 MAIN CONFERENCE SESSION CCPB 20:00– Conference banquet RHP

Sunday, January 9

08:30–17:30 Registration desk open CCPB 09:00–10:45 MAIN CONFERENCE SESSION CCPB 10:45–11:15 Coffee and posters CCPB 11:15–13:00 MAIN CONFERENCE SESSION CCPB 13:00–15:00 Lunch 15:00–16:15 MAIN CONFERENCE SESSION CCPB 16:15–16:45 Coffee and posters CCPB 16:45–19:00 MAIN CONFERENCE CLOSING SESSION CCPB 19:00–22.00 Reception and cocktail provided by the Instituto Peruano de Astronomía CAPC

Monday, January 10 – Tuesday, January 11

EXCURSION TO THE CASMA AREA

*Venues: see page 3 — 5 —

Wednesday, January 12

Time Event Venue* 08:30–17:30 Registration desk open PUCP 09:00–10:30 INTRODUCTORY WORKSHOP PUCP 10:30–11:00 Coffee and posters PUCP 11:00–13:00 REGIONAL MEETING SESSION PUCP 13:00–15:00 Lunch 15:00–16:00 REGIONAL MEETING SESSION PUCP 16:00–16:30 Coffee and posters PUCP 16:30–18:30 REGIONAL MEETING SESSION PUCP

Thursday, January 13

08:30–17:30 Registration desk open PUCP 09:00–10:30 INTRODUCTORY WORKSHOP PUCP 10:30–11:00 Coffee and posters PUCP 11:00–13:00 REGIONAL MEETING SESSION PUCP 13:00–15:00 Lunch 15:00–16:30 REGIONAL MEETING SESSION PUCP 16:30–17:00 Coffee and posters PUCP 17:00–18:30 REGIONAL MEETING SESSION PUCP

Friday, January 14

08:30–17:30 Registration desk open PUCP 09:00–10:30 INTRODUCTORY WORKSHOP PUCP 10:30–11:00 Coffee and posters PUCP 11:00–13:00 REGIONAL MEETING SESSION PUCP 13:00–15:00 Lunch 15:00–16:30 REGIONAL MEETING WORKSHOP PUCP 16:30–17:00 Coffee and posters PUCP 17:00–18:30 REGIONAL MEETING WORKSHOP PUCP

Saturday, January 15 – Tuesday, January 18

POST-CONFERENCE TOUR — INCA ARCHAEOASTRONOMY

*Venues: see page 3 — 6 —

SCIENTIFIC PROGRAMME PROGRAMA CIENTÍFICO

MAIN CONFERENCE DAY 1 (WEDNESDAY JANUARY 5): 09:00–10:00

Opening Session

09:00 Welcoming address on behalf of the Anglo-Peruvian Cultural Association by Cecilia Bentín de Cruchaga, President of the Executive Council 09:15 Welcoming address on behalf of the Pontificia Universidad Católica del Perú by Dr Efraín Gonzales de Olarte, Academic Vice-rector 09:30 Welcoming address on behalf of the International Astronomical Union by Clive Ruggles, President of Commission 41 (History of Astronomy) 09:45 Welcoming address on behalf of the International Society for Archaeoastronomy and Astronomy in Culture by Dr Stanislaw Iwaniszewski, President of ISAAC

Apertura

09:00 Discurso de Bienvenida en representación de la Asociación Cultural Peruano Británica por Cecilia Bentín de Cruchaga, Presidenta del Consejo Directivo del Británico 09:15 Discurso de Bienvenida en representación de la Pontificia Universidad Católica del Perú por Dr Efraín Gonzales de Olarte, Vicerector Académico 09:30 Discurso de Bienvenida en representación de la Unión Astronómica Internacional por Profesor Clive Ruggles, Presidente de la Comisión 41 (Historia de la Astronomía) 09:45 Discurso de Bienvenida en representación de la Sociedad Internacional para la Arqueoastronomía y Astronomía Cultural por by Dr Stanislaw Iwaniszewski, Presidente de ISAAC — 7 —

MAIN CONFERENCE DAY 1 (WEDNESDAY JANUARY 5): 10:00–13:00

General themes

Session chair: Johanna Broda (Mexico)

10:00 Opening keynote address Pushing back the frontiers or still running around the O-1 same circles? ‘Interpretative archaeoastronomy’ thirty years on Clive Ruggles (UK) 10:45 COFFEE AND POSTERS (P–1 to P–16) 11:30 Invited keynote address The two cultures of Archaeoastronomy and the History of O-2 Science Stephen McCluskey (USA) 12:15 The sky as a social field Stanislaw Iwaniszewski (Mexico) O-3 12.45 General discussion 13:00 – 15:00 LUNCH

MAIN CONFERENCE DAY 1 (WEDNESDAY JANUARY 5): 15:00–19:00

Ethnoastronomy: Case studies from South America and Australia

Session chair: Stanislaw Iwaniszewski

15:00 Invited keynote address What can the study of astronomy contribute to O-4 anthropology? An Andean perspective Gary Urton (, USA) 15:45 Palabras nuevas para viejos cielos: Formas recientes del discurso cosmológico entre O-5 aborígenes del Chaco argentino Alejandro López (Argentina) 16:15 Juventud y vejez de Dapi´chi (Pléyades): las heladas, los claveles del aire y los guerreros O-6 Cecilia Paula Gómez (Argentina) 16:45 COFFEE AND POSTERS (P–1 to P–16) 17:15 Ticuna knowledge, worecü stars and sky movements Priscila Faulhaber (Brazil) O-7 17:45 Interpretations of the Pleiades in Australian Aboriginal Dianne Johnson O-8 (Australia) 18:15 Australian Aboriginal astronomy: transient celestial phenomena Duane Hamacher and Ray O-9 Norris (Australia) 18:45 General discussion — 8 —

MAIN CONFERENCE DAY 2 (THURSDAY JANUARY 6): 09:00–13:00

Archaeoastronomy: Case studies from South America and Mesomerica

Session chair: Alejandro López 09:00 Invited student keynote address Astronomía sub-tropical en los O–10 Meridionales: el concepto de ushnu, la observación del cielo y la apropiación cultural del entorno a través de una variante del sistema de ceques en Atacama, Norte de Chile Ricardo Moyano (Mexico) 09:45 La organización espacial-calendárica y los observatorios astronómicos de O-11 Tambokancha-Zurite y Huánuco Pampa, dos asentamientos Inka como centro de Paisaje Sagrado en los Andes Centrales Jose Luis Pino Matos (Peru) 10:15 Machu Picchu and the : astronomy, ritual and imperial strategy in the Inka O-12 heartland James Farmer (USA) 10:45 COFFEE AND POSTERS (P–1 to P–16) 11:15 Can align? The enigma of Moxos´ Lagoons, astronomy and landscape in south- O-13 western Amazonia Juan Antonio Belmonte and Josep Barba (Spain) 11:45 Contributions to the study of the Muisca calendar Manuel Arturo Izquierdo (Canada) O-14 12:15 General discussion 13:00 – 15:00 LUNCH

MAIN CONFERENCE DAY 2 (THURSDAY JANUARY 6): 15:00–19:00

The 2012 Phenomenon: Maya Calendar, Astronomy, and Apocalypticism in the Worlds of Scholarship and Global Popular Culture Session organized by John B. Carlson (Center for Archaeoastronomy and the University of , College Park, Maryland, USA) and Mark Van Stone (Southwestern College, Chula Vista, California, USA)

15:00 Introduction to the session John B. Carlson & Mark Van Stone (USA) 15:45 It’s not the End of the World: emic evidence for local diversity in the Maya Long Count O-16 Mark Van Stone (USA) 16:15 Cosmogony and prophecy: Maya Era Day cosmology in the context of the 2012 O-17 prophecy Carl Callaway (Australia) 16:45 COFFEE AND POSTERS (P–1 to P–16) — 9 —

The 2012 Phenomenon (continued)

17:15 Lord of the Maya Creations on his Jaguar Throne: the eternal return of Elder Brother O-18 God L to preside over the 2012 transformation John B. Carlson (USA) 17:45 Measuring Deep Time: the sidereal year and the tropical year in Maya Inscriptions O-19 Michael J. Grofe (USA) 18:15 The God’s Grand Costume Ball: a Classic Maya prophecy for the close of the thirteenth O-20 Bak'tun Barbara MacLeod (USA) 18:45 Panel review and general discussion Led by Nicholas Campion (UK)

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PUBLIC LECTURE by Gary Urton

The Role of Khipu Cord-Keeping in Inka Astronomy, Calendrics and State Administration This talk surveys what we have learned to date about how the Inka khipu functioned as a record- keeping device and what role cord-keeping played in the construction of Inka administrative practices relating to time, materiality, and power.

CONFERENCIA PÚBLICA de Gary Urton

El Papel de los en la Astronomía Inka, los Calendarios y la Administración del Estado Esta conferencia resume lo que hemos aprendido hasta la fecha acerca de cómo los quipu inka funcionaban como dispositivos de registro y qué papel jugó el registro mediante dispositivos de cuerdas en la construcción de las prácticas administrativas inka vinculadas al tiempo, la materialidad y el poder

All Oxford IX delegates are welcome to attend this lecture, which follows the welcoming reception in the PUCP Cultural Centre, Av. Camino Real 1075, San Isidro at 21:00 on Thursday, January 6 — 10 —

MAIN CONFERENCE DAY 3 (FRIDAY JANUARY 7): 09:00–10:30

Archaeoastronomy: Case studies from Polynesia and South America

Session chair: Juan Belmonte 09:00 Invited keynote address The Polynesian ritual cycle of activities and their O-22 archaeological markers in Eastern Polynesia Edmundo Edwards (Easter Island, Chile) 09:45 Watching the sky from the ushnu: the sukanka-like summit temple in Pueblo Viejo- O-23 Pucara (Lurin Valley, Peru) Krzysztof Makowski (Peru) 10:15 General discussion 10:30 COFFEE 11:00 ONWARDS: PURUCHUCO EXCURSION

MAIN CONFERENCE DAY 4 (SATURDAY JANUARY 8): 09:00–13:00

Archaeoastronomy: Case studies from Asia

Session chair: John Steele 09:00 Cosmic capitals and numinous precincts in Early China David Pankenier (USA) O-25 09:30 Historical changes in the celebration of seasonally based holidays and festivals in Japan: O-26 a study in cultural adaptation Steven Renshaw (Japan) 10:00 A preliminary report on archaeoastronomy and ethnoastronomy in the Ryukyu Islands O-27 Akira Goto (Japan) 10:30 COFFEE AND POSTERS (P–25 to P–40) 11:00 The sun and 15 doorways of Phanom rung S. Komonjinda, A. Mullerup, L. Chunpongtong, O-28 and R. Phiromanukul (Thailand) 11:30 “Navagraha” worship: Hindu rituals for the planetary deities in the Suryanar Temple O-29 (Tamil Nadu, ). An ethnomusicological perspective Mario Friscia (Italy) 12:00 General discussion 12.30 Additional oral paper The nexus between sky and land in pre-hispanic American P–38 cultures: the role of geometry and numbers Marcello Ranieri (Italy) 13:00 – 15:00 LUNCH — 11 —

MAIN CONFERENCE DAY 4 (SATURDAY JANUARY 8): 15:00–19:00

Archaeoastronomy of the Casma Valley, Peru Session organized by Robert A. Benfer (University of Missouri, USA)

15:00 Introduction to the session Robert A. Benfer (USA) 15:30 The social and ritual context of astronomical observations at Chankillo, Casma, Peru O-31 Ivan Ghezzi (Peru) and Clive Ruggles (UK) 16:00 Chankillo: solar axis, lunar ritual, and shamanic transformation J. McKim Malville (USA) O-32 16:30 COFFEE AND POSTERS (P–25 to P–40) 17:00 Early quartz mines and other effigy mounds in the valleys of Casma and Chillón, Peru O-33 Robert A. Benfer and Larry R. Adkins (USA) 17:30 Stellar alignments in the Late Preceramic in the Casma Valley of Peru Larry R. Adkins O-34 and Robert A. Benfer (USA) 18:00 Solstice alignments in different occupation phases at Sechín Bajo Fuchs and Bernard O-35 Lorenz (USA) 18:30 Panel review and general discussion Led by Krzysztof Makowski (Peru)

MAIN CONFERENCE DAY 5 (SUNDAY JANUARY 9): 09:00–13:00

Archaeoastronomy: Case studies from the Arabic World and Europe

Session chair: Clive Ruggles 09:00 Invited keynote address Astronomy and culture in Late Babylonian Uruk John Steele O-36 (USA) 09:45 Predicting the crescent visibility with a modified astrolabe in Arabic Astronomy of X-XI O-37 centuries AD Flora Vafea (Egypt) 10:15 Ritual and the cosmos: astronomy and myth in the Athenian Acropolis Efrosyni Boutsikas O-38 (UK) and Robert Hannah (New Zealand) 10:45 COFFEE AND POSTERS (P–25 to P–40) 11:15 Archaeoastronomical research at the University of Wales, Trinity Saint David Nicholas O-39 Campion (UK) and J. McKim Malville (USA) 11:45 Diachronic study of orientations: Merida A case study César González-García and Lourdes O-40 Costa-Ferrer (Spain) 12:15 Revealing regional cultural connections within Scotland Gail Higginbottom and Andrew Smith O-41 (Australia) 12:45 General discussion 13:00 – 15:00 LUNCH — 12 —

MAIN CONFERENCE DAY 5 (SUNDAY JANUARY 9): 15:00–16:15

Archaeoastronomy: Case studies from North America

Session chair: Stephen McCluskey 15:00 Ancestors and the sun: astronomy, architecture and culture at Chaco Canyon Andrew O-42 Munro (Australia) and J. McKim Malville (USA) 15:30 Legacy documentation: using historical resources in your cultural astronomy project O-43 Gregory Munson (Colorado, USA) 16:00 General discussion 16:15 COFFEE AND POSTERS (P–25 to P–40)

MAIN CONFERENCE DAY 5 (SUNDAY JANUARY 9): 16:45–19:00

Closing Session 16:45 Commentary and discussion Presented and led by Johanna Broda (Mexico) 17:15 Portal to the Heritage of Astronomy Ruediger Schultz (Austria) O-44 17:45 ISAAC GENERAL MEETING

REGIONAL MEETING DAY 1 (WEDNESDAY JANUARY 12): 09:00–10:30

Introductory workshop I: Principles of cultural astronomy

Led by Clive Ruggles and Stanislaw Iwaniszewski 10:30 – 11:00 COFFEE AND POSTERS (P–1 to P–24)

REGIONAL MEETING DAY 1 (WEDNESDAY JANUARY 12): 11:00–17:30

Ethnoastronomy

Session chair: Priscila Faulhaber 11:00 Invited keynote address La etnoastronomía como campo académico: esbozo de un O-45 programa sudamericano Alejandro López (Argentina) 11:45 Peligro, poder y liminaridad: la luna y las mujeres Cecilia Paula Gómez (Argentina) O-46 12:15 Reflexões sobre etnoastronomia Guarani Flávia Cristina Mello, Jules Soares and Leandro O-47 Kerber (Brasil) 12:45 Discussion 13:00 – 15:00 LUNCH — 13 —

REGIONAL MEETING DAY 1 (WEDNESDAY JANUARY 12): 11:00–17:30 (continued)

15:00 Un eucalipto en la luna: folklore astronomico de los colonos europeos del norte de la O-48 provincia argentina de Santa Fe Armando Mudrik (Argentina) 15:30 La concepción Tomaraho de lo celeste Alejandro Gangui (Argentina) O-49 16:00 COFFEE AND POSTERS (P–1 to P–24) 16:30 Discussion forum Led by Alejandro López (Argentina) 17:30 – 18:30 SIAC GENERAL MEETING

REGIONAL MEETING DAY 2 (THURSDAY JANUARY 13): 09:00–10:30 Introductory workshop II: Field and laboratory techniques Led by Kim Malville and others 10:30 – 11:00 COFFEE AND POSTERS (P–1 to P–24)

REGIONAL MEETING DAY 2 (THURSDAY JANUARY 13): 11:00–16:30 Archaeoastronomy Session chair: Ricardo Moyano 11:00 Invited keynote address Ofrendas y el orden del espacio-tiempo en Mesoamerica: O-52 las matemáticas indígenas y la arqueoastronomía en una perspectiva comparativa Johanna Broda (México) 11:45 Observaciones arqueo-astronómicas en el cerro del Tepeyac: la fecha de aparición de la O-53 Virgen de Guadalupe asociado a un marcador pre-solsticial en el norte de la Cuenca de México Rafael Zimbron y Ricardo Moyano (México) 12:15 Alineamientos astronómicos del “Geoglifo de Shiqui – Jardín Jardín” sobre la meseta de O-55 Huánuco Pampa, en los Andes Centrales del Perú Jose Luis Pino Matos, Hernán Ramos Doria y Gerardo Quiroga Diaz (Perú) 12:45 Discussion 13:00 – 15:00 LUNCH 15:00 La Horca del Inca: ¿Observatorio Astronómico? Gonzalo Pereira Quiroga (Bolivia) O-56 15:30 Astronomía cultural en las laderas del volcán Galeras: Andes del sur de Colombia O-57 Armando José Quijano Vodniza (Colombia) 16:00 Discussion 16:30 – 17:00 COFFEE AND POSTERS (P–1 to P–24) — 14 —

REGIONAL MEETING DAY 2 (THURSDAY JANUARY 13): 17:00–18:30

Archaeoastronomy and education

Session chair: Ivan Ghezzi 17:00 Partiendo desde casa: educación patrimonial para la socialización del conocimiento. O-58 Arqueoastronomía de Malargüe, Mendoza, Argentina Hugo Alejandro Tucker, Roberto Bandiera, Andrés Risi, Jesica Vazquez y Karina Diaz (Argentina) 17:30 El patrimonio arqueoastronómico del Valle de Yocavil y Nevados del Aconquija en la O-59 enseñanza de la astronomía Lía Celinda Acosta y Leonor Colombo de Cudmani (Argentina) 18:00 Discussion

REGIONAL MEETING DAY 2 (THURSDAY JANUARY 13): 09:00–10:30

Introductory workshop III: South American cultural astronomy

Led by Stanislaw Iwaniszewski 10:30 – 11:00 COFFEE AND POSTERS (P–1 to P–24)

REGIONAL MEETING DAY 3 (THURSDAY JANUARY 13): 11:00–13:00

Archaeoastronomy (continued)

Session chair: Ivan Ghezzi 11:00 Calendar and agricultural regulation: solstice events in Moray, John Earls (Peru) O-61 11:45 Arqueoastronomía en el Apunao, 4753 msm, Argentina Cristian Eduardo Jacob (Argentina) O-63 12:15 Discussion forum Led by José Pino Matos (Perú)

REGIONAL MEETING DAY 2 (THURSDAY JANUARY 13): 15:00–18:30

Workshop: Cultural astronomy, film, and reporters

Organised by Jarita Holbrook and Thebe Medupe Led by Holly Wissler — 15 —

Poster papers

P–1 Ethnoastronomy and education in the Colombian Amazon Sarita Kendall, Rocio Perdomo, Marelvi Laureano and Casimiro Ahue (Colombia) P–3 Teaching archaeoastronomy and ethnoastronomy for Brazilian students from basic school Victor Alves Alencar (Brasil) P–4 Resgatando o céu através do diálogo entre a cultura científica e humanística Jules Soares, Leandro Kerber, Flávia de Mello e Romualdo Lisboa (Brasil) P–5 Una propuesta para la enseñanza de la astronomia: el recurso de la arqueoastronomia Lía Celinda Acosta, Gustavo Diaz Martin y Olga Pintado (Argentina) P–6 Visions of the Pindorama sky Rundsthen de Nader, Cintia Jales and Maura Imazio da Silveira (Brasil) P–7 Astronomy, water sources, and religion David Johnson (USA) P–8 Astronomical identity of the Inca god-creator Rita Fink (USA) P–9 Choquequirao, Topa Inca’s Machu Picchu: comparing two royal estates of the Inca Kim Malville and Gary Ziegler (USA) P–10 Límites geográficos y astronómicos del Tahuantinsuyo Barthélémy d’Ans y Manuel Aguirre-Morales (Perú) P–11 Con el sol, la luna y las estrellas: arqueoastronomia en Pachacamac Alfio Pinasco (Perú) P–12 Cuentas calendáricas en el Tawantinsuyo: una visión desde la Provincia Inca costeña de Pachacámac Juan Pablo Villanueva (Perú) P–13 Observación de los lunasticios en las culturas precolombinas Jorge Ianiszewski Rojas (Chile) P–15 Peña Horadada de Lima: descubriendo su valor arqueoastronómico Carlota Pereyra Rey (Perú) P–16 Machu Picchu: geometries, numbers and length-unit Marcello Ranieri (Italy) and Milton Rojas Gamarra (Chile) P–17 Cosmogonia indígena no Brasil e suas semelhanças nas Américas do Sul e Central Peter Leroy (Brasil) P–18 Native Brazilian astronomy Ronaldo Mourão (Brasil) P–19 El cerebro humano y la construcción del entorno: cielo y tierra como instrumento astronómico escala 1:1 Patricio Bustamante Díaz (EE.UU.) y Ricardo Moyano Vasconcellos (México) P–20 The astronomy behind the IntipRaymi ceremony Milton Rojas Gamarra and Gabriela Rojas Gamarra (Chile) P–21 Identificación de objetos astronómicos en grabados rupestres: aportes metodológicos en arqueoastronomía Hugo Tucker, Roberto Bandiera y Andrés Risi (Argentina) P–22 El cielo en las rocas: Arqueoastronomía del sur de Mendoza (Argentina) Hugo Tucker, Roberto Bandiera, Andrés Risi y Jorge Luna (Argentina) P–23 Astronomía quechua y orden celeste Barthelemy d´Ans (Perú) — 16 —

P–26 Ancient Skies: human cultures and their skies Doris Vickers and Rüdiger Schultz (Austria) P–28 Arab celestial complexes from the Pleiades to Canopus Ben Adams (USA) P–29 Traditional rites and their celestial alignments in parts of south-eastern Nigeria J.O. Urama, P. Eze-Uzomaka, F. Chami, J.K. Obatala and C. Opata (Nigeria) P–31 Astronomía, cultura y paisaje en la Edad del Hierro en la Cuenca del Ebro Manuel Pérez Gutiérrez, David Bea Castaño, Jordi Diloli Fons y Samuel Sardà Seuma (España) P–33 The astronomy of Kreisgrabenanlagen (neolithic circular ditch systems): an interdisciplinary approach Georg Zotti and Wolfgang Neubauer (Austria) P–36 Did Maya commoners build astronomically oriented architectural assemblages? Ritual site design in the suburban community of Chawak Chance Coughenour (Spain) P–37 Calendarios y Yanantín: simetrías de rotación y reflexión y diagramas espacio-temporales en América Paola González Carvajal y Javier Tamblay Sepúlveda (Chile) P–39 The astronomy of Aboriginal Australians: more than ceremony Ray Norris and Duane Hamacher (Australia) IAU S278 LIST OF PARTICIPANTS

Acosta, Lía Celinda (Argentina) [F] Adkins, Larry (USA) [M] Aguierre, Gabriela (Peru) [F] Aguirre-Morales Prouve, Manuel Augusto (Peru) [M] Alves Alencar, Victor (Brazil) [M] Araujo Camacho, Hilda (Peru) [F] Bea Castaño, David (Spain) [M] Belmonte, Juan Antonio (Spain) [M] Benfer, Robert (USA) [M] Benites Morales, Nathaly (Peru) [F] Broda, Johanna (Mexico) [F] Bustamante Diaz, Patricio Gabriel (Chile) [M] Callaway, Carl (Australia) [M] Cámara Guerrero, Jorge (Peru) [M] Campion, Nicholas (UK) [M] Carlson, John B. (USA) [M] Castillo Farroñay, Zamia (Peru) [F] Chacaltana Cortez, Sofia (Peru) [F] Chirinos Portocarrero, Ricardo (Peru) [M] Corrales, Ivan (Peru) [M] Costa Ferrer, Lourdes (Spain) [F] d´Ans, Barthelemy (Peru) [M] de Mello, Flávia Cristina (Brazil) [F] de Nader, Rundsthen (Brazil) [M] Díaz, Martín Gustavo (Argentina) [M] Diloli Fons, Jordi (Spain) [M] Dueñas Romero, Rocio del Carmen (Peru) [F] Earls, John (Peru) [M] Edwards, Edmundo (Chile) [M] Farmer, James (USA) [M] Barbosa Faulhaber, Patricia (Brazil) [F] Friscia, Mario (Italy) [M] Gangui, Alejandro (Argentina) [M] García Guzman, Giancarlo (Peru) [M] Ghezzi, Ivan (Peru) [M] Gómez, Cecilia Paula (Argentina) [F] González Carvajal, Paola (Chile) [F] González-García, A.César (Spain) [M] Goto, Akira (Japan) [M] Green, Harold H. (USA) [M] Grofe, Michael J. (USA) [M] Hamacher, Duane (Australia) [M] Hannah, Patricia (New Zealand) [F] Hannah, Robert (New Zealand) [M] Harris, Pauline (New Zealand) [F] Henríquez Barboza, Natalia Del Carmen (Chile) [F] Higginbottom, Gail (Australia) [F] Holmquist, Ulla (Peru) [F] Houston, Gordon (USA) [M] Ianiszewski Rojas, Jorge (Chile) [M] Iwaniszewski, Monica (Poland) [F] Iwaniszewski, Stanislaw (Mexico) [M] Izquierdo, Manuel Arturo (Canada) [M] Johnson, David (USA) [M] Johnson, Dianne (Australia) [F] Kaufman, Kenneth (USA) [M] Kendall, Sarita (Colombia) [F] Klokocnik, Jaroslav (Czech Republic) [M] Komonjinda, Siramas (Thailand) [F] Leavitt, Lewis (USA) [M] Lomsdalen, Tore (Italy) [M] López, Alejandro (Argentina) [M] MacLeod, Barbara (USA) [F] Makowski, Krzysztof (Peru) [M] Malville, John McKim (USA) [M] Malville, Nancy (USA) [F] Mataamua, Te Rangi (New Zealand) [M] McCluskey, Constance (USA) [F] McCluskey, Stephen (USA) [M] Medelius de Riveros, Yole (Peru) [F] Merriot, Ivy (USA) [F] Morales, Juan (Peru) [M] Moyano Vasconcellos, Ricardo F. (Mexico) [M] Mudrik, Armando (Argentina) [M] Muña Mendoza, Wilber (Peru) [M] Munizaga, Daniel (Chile) [M] Munro, Andrew (USA) [M] Munro, Anne Marie (USA) [F] Munson, Gregory (USA) [M] Napuri Peirano, Veronica (Peru) [M] Orellana Astorya, David (Chile) [M] Pajuelo Cubillas, Myriam (Peru) [F] Pankenier, David (USA) [M] Pereira Quiroga, Gonzalo (Bolivia) [M] Pereyra Rey, Carlota del Pilar (Peru) [F] Pérez Gutiérrez, Manuel (Spain) [M] Pinasco, Alfio (Peru) [M] Pino Matos, Jose Luis (Peru) [M] Pintado, Olga (Argentina) [F] Pisani, Ferdinando (Peru) [M] Quijano Vodniza, Armando José (Colombia) [M] Ranieri, Marcello (Italy) [M] Renshaw, Steven (Japan) [M] Riroroko, Mara (New Zealand) [F] Risi, Andrés (Argentina) [M] Rojas Gamarra, Milton (Chile) [M] Ruggles, Clive (UK) [M] Saez Rodriguez, Alberto (Switzerland) [M] Salas Delgado, Dante Genaro (Peru) [M] Sanhueza, Cecilia (Chile) [F] Sanz de Lara, Marguerita (Spain) [F] Schultz, Ruediger (Austria) [M] Seguil Alfonzo, Kania (Peru) [F] Skinner, Jefferson (Australia) [M] Soares, Jules (Brazil) [M] Steele, John (USA) [M] Tamblay, Javier (Chile) [M] Tello Galvez, Julio Cesar (Brazil) [M] Tucker, Hugo Alejandro (Argentina) [M] Turner, Jim (USA) [M] Urama, Johnson (Nigeria) [M] Urton, Gary (USA) [M] Vafea, Flora (Egypt) [F] Van Stone, Mark (USA) [M] Villanueva Hidalgo, Juan Pablo (Peru) [M] Vogt, Steven (USA) [M] Wissler, Holly (USA) [F] Yepes Rossel, Gabriela (Peru) [F] Zimbron, Rafael (Mexico) [M] Zotti, Georg (Austria) [M]

DISTRIBUTION BY GENDER

Male 82 68.3% Female 38 31.7%

DISTRIBUTION BY COUNTRY

Argentina 9 7.5% Australia 5 4.2% Austria 2 1.7% Bolivia 1 0.8% Brazil 6 5.0% Canada 1 0.8% Chile 10 8.3% Colombia 2 1.7% Czech Republic 1 0.8% Egypt 1 0.8% Italy 3 2.5% Japan 2 1.7% Mexico 4 3.3% New Zealand 5 4.2% Nigeria 1 0.8% Peru 29 24.2% Poland 1 0.8% Spain 7 5.8% Switzerland 1 0.8% Thailand 1 0.8% UK 2 1.7% USA 26 21.7% IAU S278 BRIEF REPORT

Overview

IAU Symposium S278, entitled “Archeoastronomy and Ethnoastronomy: Building Bridges between Cultures”, took place in Lima, Peru, on January 5–14, 2011. This was also an “Oxford” Symposium on Archeoastronomy, the ninth in what is certainly the foremost series of international conferences on the topic. Meetings in the series have been held at roughly four-yearly intervals since 1981, when Michael Hoskin, the then-Commission 41 President, organised the first.

One of the most important aspects of the conference was the strong link with the IAU’s new decadal strategic plan, “Astronomy for the Developing World”. In his opening address IAU Vice-President George Miley1 described the strategic plan as an ambitious blueprint to mobilize talented astronomers, engineers and teachers around the world in the service of developing countries. The “building bridges” of the title refers to the connections between cultural astronomy and the advancement of modern astronomy in the developing world, and the conference succeeded in sparking off several initiatives to identify and develop these connections in the coming months and years. As George pointed out: “Astronomy is a unique tool for development because it combines cutting-edge technology with fundamental science and also has deep cultural roots.” It is the business of archaeoastronomy to explore these roots.

This was the first ever IAU Symposium explicitly concerning this highly interdisciplinary topic, one of interest not only to astronomers but also to archaeologists, historians, anthropologists, architects, art historians, historians of religions and others. This was also the first “Oxford” conference to be held in South America, thus providing a unique opportunity to strengthen the community of scholars practicing ethno- and archaeoastronomy in South America and to forge stronger links between them and the global community of researchers. In order to balance global participation and regional engagement, one and a half days of the four- and-a-half-day main conference (Jan 5–9) were devoted to South American topics, while the three-day Regional Meeting (Jan 12–14) was devoted exclusively to Latin America.

The two parts of the conference attracted a total of 120 participants including 9 young Peruvian scholars and students awarded scholarships by one of the local organisers, the Anglo-Peruvian Cultural Association (ACPB). The conference attracted considerable media attention in local and national newspapers and magazines.

Scientific highlights of the meeting

One of the key characteristics of the “Oxford” conferences is the avoidance of parallel sessions, giving everyone the opportunity to hear talks by the full range of specialists, and to come into direct contact with disciplinary approaches very different from their own. The “Oxford” conferences provide a leading forum of interchange between diverse disciplines, and seven invited keynote lectures set the stage for this in Lima:

• Stephen McCluskey (USA): The two cultures of archaeoastronomy and the history of science

1 Sadly, George himself had to withdraw from the conference for health reasons, and his words were conveyed by Clive Ruggles. • Gary Urton (USA): What can the study of astronomy contribute to anthropology? An Andean perspective

• Alejandro López (Argentina): Ethnoastronomy as an academic field: the outline of a South American programme

• Johanna Broda (Mexico): Offerings and spatio-temporal order in Mesoamerica: indigenous mathematics and archaeoastronomy in comparative perspective

• Edmundo Edwards (Easter Island): The Polynesian ritual cycle of activities and their archaeological markers in Eastern Polynesia

• Ricardo Moyano (Chile): Sub-tropical astronomy in the southern Andes

• John Steele (USA): Astronomy and culture in Late Babylonian Uruk

(Unfortunately, visa problems prevented Professor Sun Xiaochun from attending the conference and presenting his keynote speech on Archaeoastronomy in China.)

Clive Ruggles’s opening keynote, “Pushing back the frontiers or still running around the same circles? ‘Interpretative archaeoastronomy’ thirty years on” ensured that cutting-edge issues of field methodology and social theory were to the fore. Archaeoastronomy is a science that addresses social questions, and it is essential not only to do meticulous science in the field but also to produce anthropologically viable interpretations.

The many highlights among the contributed papers included several on aspects of indigenous astronomical practices in Argentina, Brazil, and other South American countries; David Pankenier’s study of the cosmological design of ritual precincts in Imperial China; Efrosyni Boutsikas and Robert Hannah’s integration of evidence from archaeoastronomy and historical literature to reconstruct aspects of ancient Greek cult practices and their relationship to particular constellations; and Flora Vafea’s reconstruction, from historical accounts, of the use of a modified astrolabe to predict the visibility of the lunar crescent by tenth- and eleventh-century Muslim astronomers.

A thematic half-day session on “The 2012 phenomenon: Maya calendar, astronomy, and apocalypticism in the worlds of scholarship and global popular culture”, organized by John Carlson and Mark van Stone, linked together studies of Mayan literature and of modern “alternative” beliefs. Another on “The archaeoastronomy of the Casma Valley, Peru”, organized by Robert Benfer, provided some detailed debate about the interpretation of the now-famous thirteen towers of Chankillo, a solar observation site dating to c. 300 BC, and of related sites nearby, which was followed up by a two-day visit to the area.

A particular highlight of the conference was a public lecture by Gary Urton, Professor of Anthropology at Harvard University, entitled “The Role of Khipu Cord-Keeping in Inka Astronomy: Calendrics and State Administration”, describing how the Inka khipus (knotted-cord strings) functioned as a record-keeping device important in the maintenance of Inka administrative practices relating to time, materiality, and power. Professor Urton also provided an expert commentary on the khipus held in the museum at the Inca site of Puruchuco, visited on a half-day mid-conference excursion. IAU Symposium 279

Death of Massive Stars: Supernovae and Gamma-Ray Bursts

Nikko, Japan (Mar.12-16, 2012)

Postponed from 2011 because of the 3/11 disaster in Japan.

IAU Symposium 280 "The Molecular Universe" (May 30 - June 3, 2011, Toledo, Spain)

FINAL PROGRAM

Sunday May 29

18:00h - 21:00 Registration & Welcome reception at the Sabatini Building

Monday May 30 08:15 Registration Put up posters session 1 08:40 - 09:00 E.F. van Dishoeck Opening and welcome J. Cernicharo Logistical matters 09:00 - 09:30 A.G.G.M. Tielens The molecular universe: overview

Star Formation I (Chairs: E.F. van Dishoeck (09:30-10:45); S.-Y. Liu (11:15-11:55))

09:30 - 09:55 P. Caselli Observational studies of pre-stellar cores and IRDCs (I) 09:55 - 10:20 J. Jorgensen Interferometric studies of low-mass protostars (I) 10:20 - 10:45 Y. Aikawa Hydrodynamical-chemical models from prestellar cores to protostellar cores (I) 10:45 - 11:15 Coffee/tea 11:15 - 11:30 J.-E. Lee The D/H ratio of water ice in © 11:30 - 11:55 R. Bachiller Molecules in outflows (I)

Herschel hot results 1 (Chair: G. Pilbratt)

11:55 - 12:05 G. Pilbratt Herschel introduction 12:05 - 12:20 B. Lefloch Molecules in protostellar shocks: the CHESS view on L1157-B1 © 12:20 - 12:35 N. Crockett HEXOS: analysis of the HIFI 1.2 THz wide spectral survey toward Orion KL © 12:35 - 12:50 L. Kristensen WISHes coming true: low-mass protostars as chemical fountains © 12:50 - 13:05 A. Fuente The chemistry of water in the UC HII region MonR2 © 13:05 - 15:00 Lunch + Al Fresco discussions

Solar System Objects (Chairs: S. Charnley (15:00-16:50); G. Muñoz-Caro (16:50-17:40))

15:00 - 15:40 J. Lunine Chemistry of the Solar System (R) 15:40 - 15:55 D.E. Jennings The Atmospheres of Titan and Saturn in the IR from Cassini: The Interplay Between Observation and Lab Studies © 15:55 - 16:20 D. Bockelee-Morvan Recent results on the composition of comets (I) 16:20 - 16:35 D. Lis Herschel observations of comet Hartley 2: D/H in a Jupiter family comet © 16:35 - 16:50 M. Hogerheijde Detecting the cold water reservoir in a protoplanetary disk © 16:50 - 17:15 S. Sandford The Power of Sample Return Missions - Stardust and Hayabusa (I) 17:15 - 17:40 C. Alexander Organics in Meteorites - solar or interstellar? (I) 17:40 - 20:00 Poster session I con tapas (Poster presenters at their poster) 20:15- Buses back to hotels

IAU Symposium 280 "The Molecular Universe" Página 1 de 4 Toledo (30 mayo al 3 junio, 2011), España Tuesday May 31

Evolved Stars (Chair: D. Field)

08:45 - 09:10 S. Kwok Molecular evolution from AGB stars to planetary nebulae (I) 09:10 - 09:35 J. Cernicharo Line surveys of evolved stars (I) 09:35 - 09:50 M. Guelin Time dependent anion chemistry in the CSE IRC+10216 © 09:50 - 10:15 I. Cherchneff Molecules in supernova ejecta (I) 10:15 - 10:35 J. Cami Fullerenes in circumstellar and interstellar environments (I) 10:35 - 10:50 C.Contreras Formation and destruction processes of carbonaceous interstellar dust © 10:50 - 11:15 Coffee/tea

Star Formation and Complex Molecules (Chair: E. Herbst)

11:15 - 11:40 N. Sakai Observations of Complex Molecules in Low-Mass Protostars (I) 11:40 - 12:05 K. Oberg Ices in starless and star-forming cores (I) 12:05 - 12:30 J. Martín-Pintado GC clouds and complex molecules (I) 12:30 - 12:55 S. Widicus Models of hot cores with complex molecules (I) 12:55 - 13:10 A.I. Vasyunin New chemical models for new era observations: a multiphase Monte Carlo model of gas-grain chemistry © 13:15 - 15:15 Lunch + Al Fresco discussions Take down posters session 1 - Put up posters session 2

Basic molecular processes I (Chair: I. Sims)

15:15 - 15:55 I. Smith Gas-Phase Processes: rate coefficients, temperature dependences, and reaction products (R) 15:55 - 16:20 S. Klippenstein Theory of Low Temperature Reactions (I) 16:20 - 16:45 V. Bierbaum Anions in space and in the laboratory (I) 16:45 - 17:15 Coffee/tea

Herschel hot results 2 (Chair: J.R. Pardo)

17:15 - 17:30 P. Goldsmith Herschel oxygen project observations of O2 in Orion © 17:30 - 17:45 L. Decin Chemical enrichment of the ISM through the mass loss of evolved stars © 17:45 - 18:00 W.F. Thi Modeling the gas and dust of protoplanetary disks in the Herschel-GASPS sample © 18:00 - 18:15 S.C. Madden Where is the molecular gas in low metallicity dwarf galaxies? © 18:15 - 18:30 K.M. Menten An interferometric 270-355 GHz spectral line survey of the red supergiant VY CMa © 18:30 - 19:00 Al Fresco discussions 19:00- Buses back to hotels

IAU Symposium 280 "The Molecular Universe" Página 2 de 4 Toledo (30 mayo al 3 junio, 2011), España Wednesday June 1

Protoplanetary disks (Chair: I. Kamp)

08:45 - 09:10 A. Dutrey Millimeter/submm observations of molecules in disks (I) 09:10 - 09:25 E. Bergin DISCS: a disk imaging survey of chemistry with the SMA © 09:25 - 09:50 D. Semenov Chemical models of protoplanetary disks (I) 09:50 - 10:15 C. Salyk IR observational studies of gas in disks (I) 10:15 - 10:30 K. France The Far-UV molecular spectrum of protoplanetary disks: new views from Hubble © 10:30 - 10:55 R. Visser Chemical history of molecules in disks (I) 10:55 - 11:25 Coffee/tea

Basic molecular processes II (Chair: L. Hornekaer)

11:25 - 12:05 H. Linnartz Unlocking the (solid state) chemistry of the heavens (R) 12:05 - 12:30 F. Dulieu Water ice formation and the o/p ratio (I) 12:30 - 12:55 C. Jaeger Solid-state spectroscopy (I) 12:55 - 13:10 J.L. Lemaire Competing mechanisms in the formation of H2 on silicates in conditions pertinent to the ISM © 13:15 - 14:45 Lunch 14:45 - 17:15 Poster session 2 con café (Poster presenters at their poster)

18:00 - Buses back to hotels 20:00 - Classical Concert at Hotel Beatriz Auditorium 21:15 - Conference dinner at Hotel Beatriz

Thursday June 2

Extragalactic chemistry (Chair: S. García-Burillo)

Take down posters session 2 - Put up posters session 3 08:50 - 09:15 S. Glover The Chemistry of the Early Universe (I) 09:15 - 09:30 A. Sternberg Molecular clouds at the reionization epoch © 09:30 - 09:55 S. Muller Absorption line surveys at intermediate redshift (I) 09:55 - 10:20 S. Martin Extragalactic line surveys (I) 10:20 - 10:45 K. Kraiberg-Knudsen Observations of molecules at high redshift (I) 10:45 - 11:10 F. van der Tak Molecular data and radiative transfer (I) 11:10 - 11:40 Coffee/tea

Exoplanets and their atmospheres (Chair: G. Blake)

11:40 - 12:05 G. Tinetti Exoplanetary atmosphere observations (I) 12:05 - 12:30 E. Hebrard Exoplanetary atmosphere models (I) 12:30 - 12:45 C. Walsh The chemistry of atmospheres © 12:45 - 13:10 L. Kaltenegger Biomarkers of habitable worlds - Super- and Earths (I) 13:10 - 15:00 Lunch + Al Fresco discussions

Tools of analysis and databases (Chair: J. )

15:00 - 15:05 E. Herbst In memoriam G. Winnewisser 15:05 - 15:30 F. de Lucia How Can We Use Complete Experimental Catalogs in the Complex Spectra Limit? (I) 15:30 - 15:55 P. Schilke Tools for analysis of spectral surveys (I) 15:55 - 16:10 S. Takano Nobeyama 45m telescope legacy project: Line survey © 16:10 - 16:25 T.J. Millar Overview of data bases 16:25 - 17:30 Panel 'On to ALMA' Chair: S. Yamamoto; Panel members: G. Blake, G. Garay, M. Guelin, K. Menten 17:30 - 20:00 Poster session 3 con tapas (Poster presenters at their poster) Database demonstrations 20:15 - Buses back to hotels

IAU Symposium 280 "The Molecular Universe" Página 3 de 4 Toledo (30 mayo al 3 junio, 2011), España

Friday June 3

Diffuse clouds and PDRs (Chairs: E. Roueff (08:45-10:45); P. de Vicente (11:10-11:50))

08:45 - 09:10 E. The PAH hypothesis after 25 years (I) 09:10 - 09:25 J. Thrower Laboratory investigations of the formation of superhydrogenated PAHs © 09:25 - 09:50 N. Cox The diffuse interstellar bands and their carriers: The mystery unfolds? (I)

09:50 - 10:05 R. Raghunandan H2C3 - a diffuse interstellar band carrier © 10:05 - 10:20 G. Rouille Spectroscopy of PAHs with carbon side chains © 10:20 - 10:45 R. Meijerink PDRs and XDRs (I) 10:45 - 11:10 Coffee/tea + light snacks 11:10 - 11:35 E. Falgarone Turbulence in diffuse clouds (I) + 11:35 - 11:50 T.R. Geballe Exploring the central molecular zone with H3 and CO ©

Herschel hot results 3 (Chair: D. Johnstone)

11:50 - 12:05 J.R. Goicoechea First detection of far-IR OH emission towards the Orion Bar PDR © 12:05 - 12:25 T.G. Phillips The ubiquitous nature of HF © 12:25 - 12:40 D. Neufeld Probing the diffuse ISM with hydroxyl cations and water cations © 12:40 - 12:55 W.D. Langer Carbon chemistry in transitional clouds from the GOT C+ Survey of CII 158 micron Emission in the Galactic Plane ©

12:55 - 13:10 B. Mookerjea Herschel observations of C3 in star-forming regions ©

SUMMARY AND CLOSING

13:10 - 13:40 John Black Conference summary 13:40 - 13:50 Conference closing 13:50 - 15:15 Light lunch and Take down Posters session 3

14:30 - 16:00 Buses to Madrid Airport

Notes: (R) = Review Talk (30 + 10 min) (I) = Invited Talk (20 + 5 min) © = Contributed Talk (12 + 3 min)

LOC assistance with presentations: P. de Vicente, T. Bell and B. Godard

IAU Symposium 280 "The Molecular Universe" Página 4 de 4 Toledo (30 mayo al 3 junio, 2011), España Hoja1

PARTICIPANTS INSTITUTION COUNTRY Kinsuk Acharyya S N Bose National Centre for Basic India Sciences Gilles Adande University of U.S.A. Marcelino Agúndez Observatoire de Paris France Yuri Aikawa Kobe Univ. Japan Eiji Akiyama Ibaraki University Japan José Albaladejo Pérez Universidad de Castilla-La Mancha Spain Tobias Albertsson MPIA, Heidelberg Germany Isabel Alemán IAG-USP, University of Sao Paulo Brazil Conel Alexander Carnegie Institution of Washington. Dept. U.S.A. Terrestrial Magnet José Alonso Dpto. Química-Física e Inorgánica. Spain Facultad de Ciencias Hector Alvaro Galué FOM Rijnhuizen Netherlands Diana Andrade Universidade do Vale do Paraíba Brazil Carina Arasa Leiden Institute of Chemistry, Leiden Netherlands University Héctor Arce Yale University U.S.A. Giambattista Aresu Kapteyn Astronomical Institute Netherlands Rafael Bachiller Observatorio Astronómico Nacional Spain Gisela B. Esplugues Centro de Astrobiología Spain Bernabé Ballesteros Universidad de Castilla - La Mancha Spain Jeanette Bast Leiden Observatory Netherlands Tom Bell Centro de Astrobiología Spain Arnold Benz ETH Zurich Switzerland Alicia Berciano Alba ASTRON Netherlands Astrid Bergeat Institut des Sciences Moléculaires / France Université Bordeaux 1 Edwin Bergin University of (USA) U.S.A. Olivier Berné Leiden Observatory Netherlands Mathieu Bertin LPMAA Université Pierre et Marie Curie France Daniela Bettoni INAF - Osservatorio Astronomico di Italy Padova Ludovic Biennier Institut de Physique Univ. de Rennes France Verónica Bierbaum University of Colorado U.S.A. Thomas Bisbas University College London U.K. Chiara Biscaro Basel University Switzerland Luca Bizzocchi Centro de Astronomía e Astrofísica da Portugal Universidade de Lisboa John Black Chalmers University of Technology Sweden Sweden Geoffrey Blake Division of Geological & Planetary U.S.A. Sciences Dominique Bockelee-Morvan LESIA, Observatoire de Paris France Sylvain Bontemps LAB/OASU/Observatoire de Bordeaux France Bordeaux University Jean-Baptiste Bossa Leiden Observatory Netherlands Sandrine Bottinelli IRAP / Univ. Toulouse France

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Stefano Bovino Department of Chemistry, University of Italy Rome Sapienza Rogier Braakman Santa Fe Institute U.S.A. Wendy Brown University College London U.K. Joanna Brown Harvard-Smithsonian Center for U.S.A. Simon Bruderer MPE Garching Germany Christof Buchbender Spain Instituto de Radio Astronomía Milimétrica Gemma Busquet INAF-Istituto di Fisica dello Spazio Italy Interplanetario Denis Buechel Physical Institute: University of Cologne Germany Sylvie Cabrit LERMA - Observatoire de Paris France Jan Cami The University of Western Ontario Canada Alessandra Candian University of Nottingham U.K. André Canosa Institut de Physique de Rennes France Cristina Cappa Facultad de Ciencias Astronómicas y Argentina Geofísicas, Universidad Fabio Carelli University of Rome 'Sapienza', Italy Italy Paul Carroll Emory University U.S.A. Miguel Carvajal Universidad de Huelva Spain Paola Caselli University of Leeds U.K. Andrew Cassidy Department of and Astronomy, Denmark Aarhus University José Cernicharo CAB. INTA-CSIC Spain Qiang Chang The Ohio state University U.S.A. Germán Chaparro Molano Kapteyn Astronomical Institute Netherlands Steven Charnley NASA Goddard Space Flight Center U.S.A. Luis Chavarria LAB/OASU France Jo-Hsin Chen Jet Propulsion Laboratory / Caltech U.S.A. Isabelle Cherchneff Basel University Switzerland Jean Chiar SETI Institute U.S.A. Thierry Chiavassa Aix-Marseille University France Yunhee Choi Kapteyn Astronomical Institute / SRON Netherlands Helen Christie University College London U.K. Lauren Cleeves University of Michigan U.S.A. Claudia Comito Max-Planck-Institut fur Radioastronomie Germany Cesar Contreras NASA-Ames Research Center U.S.A. Amanda Cook NASA Ames Research Center (ORAU) U.S.A. Carla Maria Coppola Chemistry Dept (Univ. Bari)-Physics & Italy Astronomy Dept (UCL) Martin Cordiner NASA Goddard Space Flight Center U.S.A. Diane Cormier Service d'Astrophysique, CEA Saclay, France France Anne Coupeaud IRAP France Audrey Coutens IRAP France Nick Cox Institute of Astronomy, K.U.Leuven Belgium Kyle Crabtree University of Illinois U.S.A. Nathan Crockett University of Michigan U.S.A.

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Gustavo Cruz Díaz Centro de Astrobiología CSIC - INTA Spain Attila Csaszar Institute of Chemistry, Eotvos University Hungary Sara Cuadrado Prado Centro de Astrobiología (CSIC-INTA) Spain Charles Cunningham Herzberg Institute of Astrophysics Canada Herma Cuppen Institute for Molecules and Materials, Netherlands Radboud University Steven Cuylle Leiden Observatory Netherlands Alexander Dalgarno Harvard University U.S.A. Fabien Daniel CAB, INTA-CSIC Spain Ankan Das Indian Centre for Space Physics India Thijs de Graauw Joint ALMA Observatory Chile Massimo De Luca LERMA - CNRS - ENS France France Frank de Lucia Ohio State University U.S.A. Pablo de Vicente Observatorio Astronómico Nacional Spain Bernard de Vries Instituut voor Sterrenkunde, Leuven, Belgium Belgium Leen Decin Instituut voor Sterrenkunde, Leuven, Belgium Belgium Carolin Dedes Institute for Astronomy ETH Zurich Switzerland Rainer Dietsche University of Basel Switzerland Francois Dulieu LERMA. Observatoire de Paris et Univ. France Cergy Pontoise Anne Dutrey Laboratoire d'Astrophysique de Bordeaux France Yves Ellinger UPMC France Pierre Encrenaz Observatoire de Paris France Christian Endres University of Cologne Germany Sonia Erattupuzha Joseph University of Basel Switzerland Antonio Escobar Centro de Astrobiología (C.A.B-I.N.T.A) Spain Jarken Esimbek Urumqi Observatory, National China Astronomical Observatories, CAS Aaseef Esmail University of Basel Switzerland Mireya Etxaluze Centro de Astrobiología Spain Edith Falgarone LERMA/LRA. Ecole Normale Supérieure France Cecile Favre Department of Physics and Astronomy, Denmark Aarhus University Edith Fayolle Leiden Observatory Netherlands Nicole Feautrier LERMA, Paris Observatory France Gleb Fedoseev Leiden Observatory Netherlands Paul Feldman Johns Hopkins University U.S.A. Paola Fiadino Centro de Astrobiología Spain David Field University of Aarhus Denmark Jean-Hugues Fillion LPMAA, Université Pierre et Marie Curie France Nicolas Flagey Jet Propulsion Laboratory U.S.A. Francesco Fontani ESO & IRAM France Kevin France University of Colorado U.S.A. Pau Frau Institut de Ciéncies de l'Espai (IEEC-CSIC) Spain Douglas Friedel University of Illinois U.S.A. Emil Friis and Astronomy, Denmark Aarhus University

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Asunción Fuente Observatorio Astronómico Nacional Spain Kenji Furuya Kobe University, Faculty of Science Japan Giuseppe Galletta Universitá di Padova, Italy Italy Marina Galvagni Institute for Theoretical Physics, Switzerland University of Zurich Oscar Gálvez Spain Instituto de Estructura de la Materia, CSIC Yu Gao Purple Mountain Observatory China Guido Garay Universidad de Chile, Observatorio Cerro Chile Galán Santiago García-Burillo Observatorio Astronómico Nacional Spain Anibal García-Hernández Instituto de Astrofisica de Canarias (IAC) Spain Pedro García-Lario Herschel Science Centre ESAC/ESA Spain Iryna Garkusha University of Basel Switzerland Robin Garrod Cornell University U.S.A. Lisseth Gavilán Observatoire de Paris et Université de Peru Cergy-Pontoise Thomas Geballe Gemini Observatory U.S.A. Wolf Geppert Stockholm University Sweden Maryvonne Gerin LERMA France Erika Gibb University of Missouri - St. Louis U.S.A. Thomas Giesen I. Physikalisches Institut, University of Germany Cologne Simon Glover ITA/ZAH, Heidelberg Germany David Gobrecht University of Basel Switzerland Benjamín Godard Centro de Astrobiologia (CSIC-INTA) Spain Marie Godard Institut d'Astrophysique Spatiale France Javier Goicoechea Centro de Astrobilogia (CSIC-INTA) Spain Paul Goldsmith Jet Propulsion Laboratory, California U.S.A. Institute of Technolog Beatriz González García European Space Astronomy Centre (ESAC) Spain Fedor Goumans Leiden University Netherlands Pierre Gratier Institut de RadioAstronomie Millimetrique France (IRAM) Michel Guelin IRAM France Stephane Guilloteau Laboratoire d'Astrophysique de Bordeaux France Varun Gupta University of Basel Switzerland Antoine Gusdorf Max Planck Institute for Radioastronomy Germany Joseph Guss University of Leiden Netherlands Viviana Guzmán LERMA-ENS France Lizette Guzmán-Ramirez JBCA, University of Manchester U.K. Emilie Habart Institut d'Astrophysique Spatiale France Tetsuya Hama Institute of Low Temperature Science, Japan Hokkaido Univ. Mark Hammonds University of Nottingham U.K. Nanase Harada The Ohio State University U.S.A. Daniel Harsono Leiden Observatory Netherlands Tatsuhiko Hasegawa Academia Sinice Institute of Astronomy Taiwan and Astrophysics

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Eric Hébrard Laboratoire d'Astrophysique de Bordeaux France Jonathan Henshaw University of Leeds U.K. Eric Herbst The Ohio State University U.S.A. Gregory Herczeg Max-Planck-Institut für extraterrestriche Germany Physik Fabrice Herpin LAB/OASU France Cinthya Herrera Institut d'Astrophysique Spatiale France Víctor Herrero Instituto de Estructura de la Materia Spain (CSIC) Hiroshi Hidaka Institute of Low Temperature Science, Japan Hokkaido University Ugo Hincelin Laboratoire d'Astrophysique de Bordeaux- France Université Bordeaux Michiel Hogerheijde Leiden Observatory Netherlands Sacha Hony AIM/CEA-Saclay France Jiri Horacek Charles University in Institute of Czech Republic Theoretical Phys. Liv Hornekaer Aarhus University, Dept. Physics and Denmark Astronomy Subhon Ibadov Institute of Astrophysics TAS Tajikstan John Ilee The University Of Leeds U.K. Katharina Immer Max-Planck-Institut für Radioastronomie U.S.A. Natalia Inostroza CONSEJO SUPERIOR DE Spain INVESTIGACIONES CIENTIFICAS Sergio Ioppolo Leiden Observatory, Leiden University Netherlands William Irvine University of Massachusetts U.S.A. Karoliina Isokoski Leiden Observatory Netherlands Donald Jennings Goddard Space Flight Center U.S.A. Elena Jiménez Universidad de Castilla-La Mancha Spain Izaskun Jiménez-Serra Harvard-Smithsonian Center for U.S.A. Astrophysics Doug Johnstone NRC Canada, Herzberg Institute of Canada Astrophysics Jes Jorgensen Centre for Star and Planet Formation, Denmark Univ. Copenhagen Eric Josselin Laboratoire Univers & Particules de France Montpellier - Université Pavol Jusko Charles University in Prague Czech Republic Sergei Kalenskii Astro Space Center, Lebedev Physical Russia Institute Lisa Kaltenegger MPIA Germany Juris Kalvans Ventspils University College & University Latvia of Latvia Mikhel Kama University of Amsterdam, Astronomical Netherlands Institute Anton Pannekoek Inga Kamp Kapteyn Institute, University of Groningen Netherlands Agata Karska Max-Planck-Institut für extraterrestrische Germany Physik, Germany Michael Kaufman San Jose State University U.S.A. Maja Kazmierczak Nicolaus Copernicus University, Poland Poland

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Yeghis Keheyan CNR Italy Theo Khouri Universiteit van Amsterdam Netherlands Hyo Jeong Kim The University of Texas at Austin U.S.A. Stephen Klippenstein Argonne National Laboratory U.S.A. Lars Kluge I. Physikalisches Institut, University of Germany Cologne Kirsten Knudsen Chalmers University of Technology Sweden Monika Koerber I. Physikalisches Institut, University of Germany Cologne Akira Kouchi Institute of Low Temperature Science, Japan Hokkadio University Jacek Krelowski Torun Center for Astronomy N. Poland Copernicus University, Torun, Lars Kristensen Leiden Observatory Netherlands Jay Kroll Emory University U.S.A. Yi-Jehng Kuan National Taiwan Normal University Taiwan Sun Kwok The University of Hong Kong China Jacob Laas Emory University U.S.A. Fred Lahuis SRON Netherlands Institute for Space Netherlands Research Julien Lambert Laboratoire Univers & Particules de France Montpellier - Université Thanja Lamberts Leiden Observatory, University of Leiden Netherlands William Langer Jet Propulsion Laboratory (Caltech) U.S.A. Grigorii Larionov Astro Space Center of Lebedev Physical Russia Institute. Franck Le Petit LUTH - Paris Observatory France Sébastien Le Picard Institut de Physique de Rennes, Université France de Rennes 1 Dae-Hee Lee Korea Astronomy and Space science South Korea Institute Jeong-Eun Lee Kyung Hee University South Korea Bertrand Lefloch IPAG France Jean Louis Lemaire Observatoire de Paris & Université de France Cergy-Pontoise Pierre Lesaffre CNRS,LERMA/ENS/LRA France Silvia Leurini MPIfR Germany Francois Levrier LERMA-ENS France Xiaohu Li Leiden Observatory Netherlands Johan Lindberg Centre for Star and Planet Formation Denmark University of Copenhag Harold Linnartz Leiden Observatory, Sackler Laboratory Netherlands for Astrophysics Dariusz Lis California Institute of Technology U.S.A. Sheng-Yuan Liu Academia Sinica, Institute of Astronomy Taiwan and Astrophysics Alexandra Lockwood California Institute of Technology U.S.A. Edo Loenen Leiden Observatory Netherlands Jean-Christophe Loison IS - Université de Bordeaux 1 - CNRS France

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Robin Lombaert Instituut voor Sterrenkunde KULeuven Belgium Savino Longo Dept Chemistry Univ. - IIP CNR Bari Italy Juan López Universidad de Valladolid Spain Ana López-Sepulcre IPAG - Grenoble France Jonathan Lunine The University of Arizona. Dept. of U.S.A. Planetary Sciences Roxana Lupu University of U.S.A. James Lyons UCLA U.S.A. Suzanne Madden CEA, Saclay SAp France José Madiedo UNIVERSITY OF HUELVA Spain Jean-Pierre Maillard Institut d'Astrophysique de Paris France Liton Majumdar Indian Centre for Space Physics India Margot Mandy University of Northern British Columbia Canada Nuria Marcelino National Radio Astronomy Observatory U.S.A. Sergio Martín European Southern Observatory Chile Jesús Martín-Pintado Centro de Astrobiologia (CSIC-INTA) Spain Belén Maté Instituto de Estructura de la Materia, Spain CSIC. Christopher Materese SETI U.S.A. Rainer Mauersberger Joint ALMA Observatory Chile Carolyn McCoey University of Waterloo Canada Daniel McElroy Queen's University Belfast Northern Ireland Brett McGuire Emory University U.S.A. Alan McLoughlin Queen's University Belfast U.K. Gwendolyn Meeus Universidad Autónoma de Madrid, Spain Spain Tom Megeath University of Toledo U.S.A. Rowin Meijerink Leiden Observatory Netherlands Gary Melnick Harvard-Smithsonian Center for U.S.A. Astrophysics Vito Mennella INAF-Osservatorio Astronomico di Italy Capodimonte Karl Menten Max-Planck-Institut für Radioastronomie Germany Pablo Merino-Mateo Centro de Astrobiología INTA-CSIC Spain Elisabetta Micelotta CRESST/USRA/NASA Goddard Space U.S.A. Flight Center Stefanie Milam NASA Goddard Space Flight Center U.S.A. Tom Millar Queen's University Belfast U.K. Faviola Molina Institute for Theoretical Astrophysics, Germany Heidelberg Universit Raquel Monje California Institute of Technology U.S.A. Julien Montillaud IRAP - Toulouse, France France Thierry Montmerle Institut d'Astrophysique de Paris France Bhaswati Mookerjea Tata Institute of Fundamental Research India Oscar Morata ASIAA Taiwan Stefanie Muehle Joint Institute for VLBI in Europe Netherlands Sebastien Muller Onsala Space Observatory Sweden Guillermo Muñoz Caro Centro de Astrobiología (CAB), Spain INTA/CSIC Andra Muntean Queen`s University Belfast U.K.

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Holger Müller I. Physikalisches Institut Universitát zu Germany Köln Zsofia Nagy Kapteyn Astronomical Institute & SRON Netherlands Adam Nagy University of Basel Switzerland Binukumar Nair The Open University, UK U.K. Tac Nakajima National Astronomical Observatory of Japan Japan David Neufeld Johns Hopkins University U.S.A. Hideko Nomura Kyoto University Japan Michel Nuevo NASA Ames Research Center (SETI) U.S.A. Yasuhiro Oba Institute of Low Temperature Science, Japan Hokkaido Univ. Karin Oberg Harvard-Smithsonian Center for U.S.A. Astrophysics Angela Occhiogrosso University College of London (UCL) U.K. Hans Olofsson Onsala Space Observatory Sweden Volker Ossenkopf I. Physikalisches Institut der Universitát zu Germany Köln Susana Pacheco Vázquez (IPAG) Institut de Planétologie et France d'astrophysique de Greno Laurent Pagani LERMA & UMR8112 Observatoire de Paris France & CNRS Aina Palau Institut de Ciéncies de l'Espai (CSIC-IEEC) Spain Maria Elisabetta Palumbo INAF - Osservatorio Astrofisico di Catania Italy Juan Pardo Centro de Astrobiología (INTA-CSIC) Spain Andrey Paska The University of Manchester U.K. Francoise Pauzat CNRS/UPC France John Pearson Jet Propulsion Laboratory, California U.S.A. Institute of Technology Els Peeters University of Western Ontario \& SETI Canada Institute Yezhe Pei Ohio State University U.S.A. Ruisheng Peng Caltech Submillimeter Observatory U.S.A. Tzu-Cheng Peng Laboratoire d'Astrophysique de Bordeaux France Juan-Pablo Pérez-Beaupuits Max-Planck Institut für Radioastronomie Germany Francisco Pérez-Bernal Universidad de Huelva Spain Amélie Pernet UPC France Magnus Persson Centre for Star and Planet Formation, Denmark Copenhagen University Carina Persson Onsala space observatory, Chalmers Sweden University of Technology Dawn Harvard-Smithsonian Center for U.S.A. Astrophysics Andreea Petric Caltech U.S.A. Annemieke Petrignani Leiden Observatory Netherlands Thomas Phillips California Institute of Technology U.S.A. Göran Pilbratt ESA Astrophysics issions Div / Research Netherlands and Scientific Sup Paolo Pilleri Observatorio Astronomico Nacional Spain

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Sergio Pilling UNIVAP Brazil Julien Pilme Laboratoire de Chimie Théorique. UPC France Nuria Pinol Ferrer Department of Astronomy, Stockholm Sweden University Ciro Pinto SRON - Netherlands Institute for Space Netherlands Research Claire Pirim LADIR UMR 7075/CNRS UPMC France Rene Plume University of Calgary Canada Linda Podio Kapteyn Astronomical Institute Netherlands Thomas Posch University of Wien Austria Fabrizio Puletti University College London U.K. Guillermo Quintana-Lacaci Instituto de Radioastonomía Milimétrica Spain Mary Radhuber Emory University U.S.A. Ranjini Raghunandan University of Basel Switzerland Mark Rawlings Joint ALMA Observatory Chile Pilar Redondo Universidad de Valladolid Spain Miguel Requena Torres Max-Planck-Institute für Radioastronomie Germany Anita Richards UK ALMA Regional Centre, JBCA, U.K. University of Manchester Paul Rimmer Ohio State University U.S.A. Denise Riquelme IRAM, Spain Spain Victor M. Rivilla Centro de Astrobiología INTA-CSIC Spain Ricardo Rizzo Centro de Astrobiologia Spain Julia Roberts Centro de Astrobiología (INTA/CSIC) Spain Arturo Rodríguez Franco Centro de Astrobiología CSIC-INTA Spain Evelyne Roueff Observatoire de Paris France Gaël Rouillé Universitát Jena - Max-Planck-Institut für Germany Astronomie Georgij Rudnitskij Sternberg Astronomical Institute, Moscow Russia State University Nicola Sacchi INAF-IFSI Italy Alfonso Sáiz López Laboratorio de Ciencias de la Atmósfera y Spain el Clima (CIAC) Nami Sakai The University of Tokyo Japan Takeshi Sakai The University of Tokyo Japan Farid Salama NASA-Ames Research Center U.S.A. Dinalva Sales UFRGS - Universidade Federal do Rio Brazil Grande do Sul Francisco Salgado Leiden Observatory Netherlands Colette Salyk University of Texas at Austin, McDonald U.S.A. Observatory Irene San José García Leiden Observatory Netherlands Carmen Sánchez Contreras Astrobiology Center Spain Álvaro Sánchez-Monge INAF-Osservatorio Astrofisico di Arcetri Italy Scott Sandford NASA-Ames Research Center U.S.A. Gina Santangelo INAF - Osservatorio Astronomico di Roma Italy Arkaprabha Sarangi Basel University Switzerland Peter Sarre The University of Nottingham U.K.

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Peter Schilke I. Physikalisches Institut der Universitát zu Germany Köln Eric Schindhelm University of Colorado U.S.A. Stephan Schlemmer I. Physikalisches Institut, Universitát zu Germany Köln Miroslaw Schmidt Nicolaus Copernicus Poland Nicola Schneider CEA Saclay France Dmitry Semenov Max Planck Institute of Astronomy, Germany Heidelberg María Luisa Senent Díez Spain Instituto de Estructura de la Materia, CSIC Bethmini Senevirathne University of Gothenburg Sweden Sachindev Shenoy NASA Ames Research Center U.S.A. Takashi Shimonishi Department of Astronomy, Graduate Japan School of Science Ivar Shmeld Ventspils University College, VIRAC Latvia Ian Sims Universite de Rennes1 France Howard Smith Harvard-Smithsonian Cente for U.S.A. Astrophysics Ian Smith U.K. Rachel Smith University of California, Los Angeles U.S.A. Theodore Snow University of Colorado U.S.A. Amiel Sternberg Tel Aviv University Israel Yu-Nung Su Academia Sinica, Institute of Astronomy Taiwan and Astrophysics Ewelina Szymanska The Open University U.K. Marian Szymczak Torun Centre for Astronomy, Nicolaus Poland Copernicus University Mario Tafalla Observatorio Astronómico Nacional Spain Shuro Takano Nobeyama Radio Observatory, National Japan Astronomical Observator Dahbia Talbi LUPM CNRS/Université de Montpellier II France Jonathan Tan University of Florida U.S.A. Vianney Taquet Institut de Planétologie et d'Astrophysique France de Grenoble Konstantinos Tassis Jet Propulsion Laboratory / Caltech U.S.A. Belén Tercero CAB. INTA-CSIC Spain David Teyssier ESAC Spain Patrice Theule University of Provence France Wing-Fai Thi Institut de Planetologie et d'Astrophysique France de Grenoble Sven Thorwirth I. Physikalisches Institut Universitát zu Germany Köln John Thrower Aarhus University Denmark Alexander Tielens Leiden Observatory Netherlands University College London. Dept. of U.K. Physics and Astronomy Samuel Tisi Department of Physics and Astronomy, Canada University of Waterloo

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Thomas Townsend Universidad de Castilla- La Mancha Spain Josep Trigo Rodríguez Institute of Space Sciences (CSIC-IEEC) Spain Matthew Troutman University of Missouri - St. Louis U.S.A. Antonio Usero Observatorio Astronómico Nacional Spain Nathalie Vaeck Université Libre de Bruxelles Belgium Nienke van der Marel Leiden Observatory Netherlands Floris van der Tak SRON Netherlands Ewine van Dishoeck Leiden Observatory/PE Netherlands Peter van Hoof Royal Observatory of Belgium Belgium Huib Jan van Langevelde Joint Institute for VLBI in Europe and Netherlands Sterrewacht Leiden, Magda Vasta INAF OA Arcetri - Florence Italy Charlotte Vastel IRAP/Université de Toulouse France Anton Vasyunin The Ohio State University U.S.A. Tatiana Vasyunina The Ohio State University U.S.A. Luis Velilla Prieto CAB (Astrobiology Center). INTA-CSIC. Spain Thangasamy Velusamy Jet Propulsion Laboratory (Caltech) U.S.A. Gianfranco Vidali Syracuse University U.S.A. Ruud Visser University of Michigan U.S.A. Serena Viti Department of Physics and Astronomy, U.K. University College Lond Stéphane Vranckx Free University of Brussels (ULB) Belgium Valentine Wakelam Laboratoire d'Astrophysique de France Bordeaux / Université de Bord Malcolm Walmsley INAF-Osservatorio di Arcetri Italy Catherine Walsh Queen's University Belfast U.K. Adam Walters IRAP France Susanne Wampfler Institute for Astronomy, ETH Zurich Switzerland Kuo-Song Wang Leiden Observatory Netherlands Naoki Watanabe Institute of Low Temperature Science, Japan Hokkaido Univ. Yoshimasa Watanabe The University of Tokyo Japan Susanna Widicus Weaver Emory University U.S.A. Dmitri Wiebe Institute of Astronomy of the RAS Russia Eva Wirström NASA Goddard Space Flight Center U.S.A. Markus Wittkowski ESO Germany Mark Wolfire University of Maryland U.S.A. Paul Woods University College London U.K. Bohan Wu University of Basel Switzerland Ronin Wu Service d'Astrophysique CEA Saclay France Friedrich Wyrowski Max Planck Institute for Radioastronomy, Germany Bonn Satoshi Yamamoto Department of Physics, The University of Japan Tokyo Umut Yildiz Leiden Observatory Netherlands Walter Yvart LERMA France Laimons Zacs University of Latvia Latvia Junfeng Zhen Sackler laboratory for astrophysics, Leiden Netherlands Observatory

Página 11 Hoja1 jianjun Zhou Urumqi Observatory, National China Astronomical Observatories, CAS Igor Zinchenko Institute of Applied Physics, Russian Russia Academy of Sciences Emilie-Laure Zins LADIR Université Pierre et Marie Curie France

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INTERNATIONAL ASTRONOMICAL UNION

UNION ASTRONOMIQUE INTERNATIONALE

IAU Symposium 280

Toledo, Spain 30 May – 3 June 2011

REPORT

Over 400 participants from 30 countries gathered in Toledo, Spain to attend IAU Symposium 280, entitled “The Molecular Universe,” which took place from 30 May – 3 June 2011 at the Technological Campus of the University of Castilla-La Mancha in Toledo, Spain. This is the main worldwide conference in the field of astrochemistry, held every ~5 years, and covering all areas in which molecules are found, from Solar system to the highest redshift galaxies. This breadth of topics sets the IAU symposia series apart from other meetings in the field. The weather was mainly sunny but not overly hot, allowing for many informal outdoor interactions. The Local Organizing Committee, chaired by J. Cernicharo, who was assisted by R. Bachiller, organized both the scientific and structural aspects of the meeting very well, including a delightful banquet and preceding concert. Almost all possible problems were handled amicably by M. Castellanos before the meeting was held. The cultural mecca that is Toledo added a sense of awe and excitement to the symposium, and was very easy to reach by rapid train from Madrid. The large size of the meeting did not interfere with the proceedings in any way; the auditorium where the talks were held was large enough for all participants, and the audio and video systems operated quite well. A large number of questions were asked of speakers, who, given their relative youth and diversity, brought many different viewpoints to the proceedings. The three dedicated 2.5-hr. poster sessions were very well attended and enriched the experience of the participants. The sessions were enlivened by tapas and by a variety of beverages. Informal conversations, held at intermissions from the speaking program, and during the poster sessions, were many and spirited. The large number of younger scientists at the meeting was quite impressive, and confirmed that the field of astrochemistry is entering a period of rapid growth led by new and exceedingly powerful telescopes. Whether the next meeting in the series of IAU symposia on astrochemistry can be held in the same format or will require at least some multiple sessions remains to be seen and depends upon whether the growth in size from one symposium to the next continues to occur.

The scientific organization of the symposium was undertaken by a very active IAU Working Group on Astrochemistry, under the sponsorship of IAU Commission 34 (Division VI), with co- sponsorship provided by Division VI (Interstellar Matter), Division VIII (Galaxies and the Universe), Division X (Radio Astronomy) as well as Commissions 51 (Bio-astronomy), 36 (Theory of Stellar Atmospheres), and 14 (Atomic and Molecular Data). In addition to funds from the IAU, the symposium was supported by the Spanish Ministry of Science and Innovation and the University of Castilla – La Mancha as well as by the personal research funds of J. Cernicharo (Head, LOC) and funds from his institute. There have now been six IAU symposia on astrochemistry, starting with the one held in India (1985; IAU Symposium 120). Later meetings in the series were held in Brazil (1991; IAU Symposium 150), the Netherlands (1996; IAU Symposium 178); South Korea (1999; IAU Symposium 197), and California, USA (2005; IAU Symposium 231). Each symposium has been larger than its predecessor, showing that astrochemistry is becoming a larger and more diverse community.

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The scientific program of the symposium was divided into three parts: invited and review talks, contributed talks, and poster presentations. The Scientific Organizing Committee, which was the Working Group on Astrochemistry, democratically elected the speakers who gave contributed talks among the many applicants. Overall, there were 41 invited and review talks, 32 contributed talks, and 323 posters. In the oral program were three sessions on new results from the Herschel Space Observatory labeled “Herschel hot results,” as well as a panel discussion entitled “On to ALMA.” The panel members adjudicated a contest in which young investigators competed to win a prize for the best and next best projects for ALMA with the constraint of at most 10 hours observing time. There were three large poster sessions, and awards were given to the best posters in each of the three from personal funds by E. van Dishoeck. During the third poster session, there were also computer demonstrations of databases. The abstracts for all contributions to the symposium can be found on the NASA Astrophysics Data System and on the conference website: http://www.cab.inta- csic.es/molecular_universe/show-abstracts.php, where actual poster presentations have been uploaded by many of the authors. For those of you who prefer videos, a number of interviews and highlights of the three poster sessions can be found on the IAU Symposium 280 YouTube Channel (http://www.youtube.com/user/IAUsymposium280). Invited and review talks will appear in the symposium volume, edited by J. Cernicharo and R. Bachiller.

After brief words of welcome by E. van Dishoeck, chair of the SOC, and J. Cernicharo, chair of the LOC, the 4.5-day oral program started with a general introduction on the molecular universe by A. Tielens, which was followed by a session on star formation. This field has become broader since the last astrochemistry symposium, and observational talks concerning stages of both low-mass and high-mass star formation were given, as was a theoretical talk on a new class of models that combine hydrodynamics with chemical simulations in the formation of protostellar cores. This session was followed by the first session of hot results from Herschel, which emphasized observations of water vapor, molecules in protostellar shocks, and a wide spectral survey toward Orion KL.

Astrochemistry certainly extends to planetary studies, including solar system objects. A session on these objects was held after lunch on the first day of the meeting, starting with a review talk on the chemistry of the solar system, including the origin of water on , which was followed by talks on comets, meteorites, and the atmospheres of Titan and Saturn. The power of sample return missions to solar system bodies was emphasized.

The second day of the meeting started with a session on evolved stars, in which supernova chemistry was also discussed. Talks on the molecular evolution from AGB stars to planetary nebulae, the role of time-dependent anionic chemistry (involving negatively-charge molecules) in IRC+10216, and the detection of fullerenes in assorted environments rounded out the session. Complex molecules are well known in IRC+10216 and other selected circumstellar sources, so this session merged well with the next one on star formation and complex molecules. Here observations of complex molecules were discussed in a variety of objects, along with current gas-grain simulations as well as possible future simulations involving the use of stochastic methods to improve the surface chemistry occurring in granular icy mantles.

Astrochemistry is based on the laboratory and theoretical study of basic atomic and molecular processes, and two sessions were held on this subject. The first concerned gas-phase processes, where a review talk was given on gas-phase reactions as a function of temperature, followed by a talk concerning the theory of low-temperature reactions, and one on experimental studies on the rates of reactions involving anions and how they relate to the observations of such species in various sources. The second day of the meeting ended with another Herschel hot topic session, highlighted by the report of an unambiguous detection of molecular oxygen in the interstellar medium.

The topic of protoplanetary disks occupied the first group of speakers on Wednesday, with talks on the phenomenal developments in observations at a variety of wavelengths ranging from the

! 2! ! millimeter to the far-UV and an emphasis on interferometry. Modeling was also discussed, as was the chemical history of molecules from the hot core to the disk stage. Another session on basic molecular processes followed, this one emphasizing surface processes in the laboratory and in space. Much progress has been made during the last decade in this field, but there is still a great need for further laboratory studies before robust interstellar chemical simulations including surface processes can be constructed.

Although most of astrochemistry still revolves around galactic sources, the field of extragalactic astrochemistry will receive a big boost with the onset of ALMA observations. So, it was quite appropriate to have a session on extragalactic astrochemistry, which was held on Thursday morning. This field was understood to include the early universe, so talks on early chemistry were included along with a talk on extragalactic line surveys. It is impressive to see spectra of extragalactic sources with similar complexity to those found in galactic star-forming regions three decades ago! Next in line was the explosive topic of and their atmospheres, which will occupy more and more astrochemists as more is learned about planetary atmospheres. Talks on observations, atmospheric models and their chemistry, as well as biomarkers of habitable worlds were included. The inclusion of astrobiology is a sign that this field is gaining importance and certainly overlaps with areas of astrochemistry such as the formation of complex molecules. The final session on Thursday concerned the tools of analysis and databases. Starting with a brief memorial to the late astronomer and astrochemist Gisbert Winnewisser, this session included talks on how to reduce the problem of unidentified lines in hot cores, on various tools for analysis of spectral surveys, on a legacy line survey from the Nobeyama telescope, and on databases and their uses. The session ended with the panel discussion discussed previously.

The last day of the symposium started with a session nominally on diffuse clouds and photon- dominated regions (PDRs). The role of turbulence in diffuse clouds was discussed, as was a controversial candidate for a carrier of several diffuse interstellar bands (H2C3). A talk on both PDRs and XDRs (X-ray dominated regions) was given as was a more general talk on diffuse interstellar bands. A number of aspects of the PAH hypothesis were touched upon. Finally, the complex nature of the central molecular zone of our galaxy, as seen through the infra-red spectrum of H3+, was explored. Next came the third of the Herschel hot topic sessions, which included talks on observations of diffuse clouds in the spiral arms of the Milky Way, carbon chemistry in translucent clouds, and the detection of C3 in envelopes of star-forming regions. The detection of the reactive ions OH+ and H2O+ in a variety of sources was an exceptionally interesting topic. The oral program was concluded with an exceedingly thoughtful summary of the field, past, present, and future, by J. Black.

The reader of the written volume can expect to find a cornucopia of riches concerning the state of astrochemistry before the fundamental changes that will occur when observations using the ALMA interferometer add greatly to our knowledge of sources throughout the universe. By the time of the next astrochemical symposium, much progress will have been made and the field will have grown both in size and, we trust, in understanding.

Eric Herbst

Secretary, SOC

! 3! REPORT OF ACTIVITIES WORKING GROUP ON ASTROCHEMISTRY DIVISION VI (INTERSTELLAR MATTER) COMMISSION 34 The current working group on astrochemistry has performed one of its last major functions in planning IAU Symposium 280,“The Molecular Universe” which was held in late May to early June in Toledo, Spain. In the near future, a new working group will be constituted with Tom Millar (Queens University Belfast, Northern Ireland, president) and Satoshi Yamamoto (University of Tokyo, Japan) Secretary. The working group has also proposed an upgrade of the group to a Commission on Astrochemistry. Over 435 participants from 31 countries gathered in Toledo, Spain to attend IAU Symposium 280, which took place from 30 May to 3 June 2011 at the Technological Campus of the University of Castilla-La Mancha in Toledo, Spain. This symposium is the main worldwide conference in the field of astrochemistry, held every 5 years, and covering all areas in which molecules are found, ⇠ from the Solar System to the highest redshift galaxies. The Local Organizing Committee, chaired by J. Cernicharo and R. Bachiller, organized both the scientific and structural aspects of the meeting very well. Almost all possible logistic problems were handled amicably by M. Castellanos together with the other members of the LOC. The cultural mecca that is Toledo added a sense of awe and excitement to the symposium. The large size of the meeting did not interfere with the proceedings in any way. A large number of questions were asked of speakers, who, given their relative youth and diversity, brought many di↵erent viewpoints to the discussions. The three dedicated 2.5-hr. poster sessions were very well attended and enriched the experience of the participants. Informal conversations, held at intermissions from the speaking program, and during the poster sessions, were many and spirited. The large number of younger scientists at the meeting was quite impressive, and confirmed that the field of astrochemistry is entering a period of rapid growth led by new and exceedingly powerful telescopes. The scientific organization of the symposium was undertaken by a very active IAU Working Group on Astrochemistry, under the sponsorship of IAU Commission 34 (Division VI), with co-sponsorship provided by Division VI (Interstellar Matter), Division VIII (Galaxies and the Universe), Division X (Radio Astronomy) as well as Commissions 51 (Bio-astronomy), 36 (Theory of Stellar Atmospheres), and 14 (Atomic and Molecular Data). There have now been six IAU sym- posia on astrochemistry, starting with the one held in India (1985; IAU Symposium 120). Later meetings in the series were held in Brazil (1991; IAU Symposium 150), the Netherlands (1996; IAU Symposium 178); South Korea (1999; IAU Symposium 197), and California, USA (2005; IAU Symposium 231). Each symposium has been larger than its predecessor, showing that astro- chemistry is becoming a larger and more diverse community. The scientific program of the symposium was divided into three parts: invited and review talks, contributed talks, and poster presentations. The Scientific Organizing Committee, which was the Working Group on Astrochemistry, democratically elected the speakers who gave contributed talks among the many applicants. Overall, there were 42 invited and review talks, 32 contributed talks, and nearly 360 posters. In the oral program were three sessions on new results from the Herschel Space Observatory labeled Herschel hot results, as well as a panel discussion entitled On to ALMA. The panel members adjudicated a contest in which young investigators competed to win a prize for

1 the best and next best projects for ALMA with the constraint of at most 10 hours observing time. There were three large poster sessions, and awards were given to the best posters in each of the three from personal funds by E. van Dishoeck. During the third poster session, there were also computer demonstrations of databases. After brief words of welcome by E. van Dishoeck, chair of the SOC, and J. Cernicharo, chair of the LOC, the 4.5-day oral program started with a general introduction on the molecular universe by A. Tielens, which was followed by a session on star formation. This field has become broader since the last astrochemistry symposium, and observational talks concerning stages of both low- mass and high-mass star formation were given, as was a theoretical talk on a new class of models that combine hydrodynamics with chemical simulations in the formation of protostellar cores. This session was followed by the first session of hot results from Herschel, which emphasized obser- vations of water vapor, molecules in protostellar shocks, and a wide spectral survey toward Orion KL. Astrochemistry certainly extends to planetary studies, including solar system objects. A ses- sion on these objects was held on the first day of the meeting, starting with a review talk on the chemistry of the solar system, including the origin of water on Earth, which was followed by talks on comets, meteorites, and the atmospheres of Titan and Saturn. The power of sample return missions to solar system bodies was emphasized. The second day of the meeting started with a session on evolved stars, in which supernova chemistry was also discussed. Talks on the molecu- lar evolution from AGB stars to planetary nebulae, the role of time-dependent anionic chemistry (involving negatively-charge molecules) in IRC+10216, and the detection of fullerenes in assorted environments rounded out the session. Complex molecules are well known in IRC+10216 and other selected circumstellar sources, so this session merged well with the next one on star forma- tion and complex molecules. Here observations of complex molecules were discussed in a variety of objects, along with current gas-grain simulations as well as possible future simulations involving the use of stochastic methods to improve the surface chemistry occurring in granular icy mantles. Astrochemistry is based on the laboratory and theoretical study of basic atomic and molecular processes, and two sessions were held on this subject. The first concerned gas-phase processes, where a review talk was given on gas-phase reactions as a function of temperature, followed by a talk concerning the theory of low-temperature reactions, and one on experimental studies on the rates of reactions involving anions and how they relate to the observations of such species in various sources. The second day of the meeting ended with another Herschel hot topic session, highlighted by the report of an unambiguous detection of molecular oxygen in the interstellar medium. The topic of protoplanetary disks occupied the first group of speakers on Wednesday, with talks on the phenomenal developments in observations at a variety of wavelengths ranging from the millimeter to the far-UV and an emphasis on interferometry. Modeling was also discussed, as was the chemical history of molecules from the hot core to the disk stage. Another session on basic molecular processes followed, this one emphasizing surface processes in the laboratory and in space. Much progress has been made during the last decade in this field, but there is still a great need for further laboratory studies before robust interstellar chemical simulations including surface processes can be constructed. Although most of astrochemistry still revolves around galactic sources, the field of extragalactic astrochemistry will receive a big boost with the onset of ALMA observations. So, it was quite ap-

2 propriate to have a session on extragalactic astrochemistry, which was held on Thursday morning. This field was understood to include the early universe, so talks on early chemistry were included along with a talk on extragalactic line surveys. It is impressive to see spectra of extragalactic sources with similar complexity to those found in galactic star-forming regions three decades ago! Next in line was the explosive topic of exoplanets and their atmospheres, which will occupy more and more astrochemists as more is learned about planetary atmospheres. Talks on observations, atmospheric models and their chemistry, as well as biomarkers of habitable worlds were included. The inclusion of astrobiology is a sign that this field is gaining importance and certainly overlaps with areas of astrochemistry such as the formation of complex molecules. The final session on Thursday con- cerned the tools of analysis and databases. Starting with a brief memorial to the late astronomer and astrochemist Gisbert Winnewisser, this session included talks on how to reduce the problem of unidentified lines in hot cores, on various tools for analysis of spectral surveys, on a legacy line survey from the Nobeyama telescope, and on databases and their uses. The session ended with the panel discussion discussed previously. The last day of the symposium started with a session nominally on di↵use clouds and photon- dominated regions (PDRs). The role of turbulence in di↵use clouds was discussed, as was a con- troversial candidate for a carrier of several di↵use interstellar bands (H2C3). A talk on both PDRs and XDRs (X-ray dominated regions) was given as was a more general talk on di↵use interstellar bands. A number of aspects of the PAH hypothesis were touched upon. Finally, the complex nature + of the central molecular zone of our galaxy, as seen through the infra-red spectrum of H3 , was explored. Next came the third of the Herschel hot topic sessions, which included talks on observa- tions of di↵use clouds in the spiral arms of the Milky Way, carbon chemistry in translucent clouds, and the detection of C3 in envelopes of star-forming regions. The detection of the reactive ions + + OH and H2O in a variety of sources was an exceptionally interesting topic. The oral program was concluded with an exceedingly thoughtful summary of the field, past, present, and future, by J. Black. The reader of this volume will find a cornucopia of riches concerning the state of astrochemistry before the fundamental changes that will occur when observations using the ALMA interferometer add greatly to our knowledge of sources throughout the universe. By the time of the next astro- chemical symposium, much progress will have been made and the field will have grown both in size and, we trust, in understanding. CURRENT MEMBERS OF THE WORKING GROUP ON ASTROCHEMISTRY E. van Dishoeck (President, The Netherlands) E. Herbst (Secretary, USA) Y. Aikawa (Japan) J. Black (Sweden) G. A. Blake (USA) P. Caselli (United Kingdom) J. Cernicharo (Spain) G. Garay (Chile) M. Guelin (France) U. Jorgensen (Denmark) S. Kwok (China) J. Maier (Switzerland) K. Menten (Germany) T. Millar (United Kingdom) F. Salama (USA) I. Sims (France) A. Sternberg (Israel)

Eric Herbst Secretary, Scientific Organizing Committee September 2011

3

IAU SYMPOSIUM 281

“BINARY PATHS TO TYPE IA SUPERNOVAE EXPLOSIONS”

PADOVA, ITALY, JULY 4-8 281

Only the name of the presenter is given here – Pleaese check Abstract Booklet for a ful list of authors.

SUNDAY JULY 3

18.30 Wine and Cheese reception and Castle visit at INAF-Padova

REGISTRATION TABLE OPEN AT INAF

MONDAY JULY 4

REGISTRATION TABLE OPEN AFTER 8.15 am

9-9.55 INTRODUCTION

9-9.15 Marina Orio – INAF-PD Director - Padova mayor - 5 min each "Welcome addresses"

9.15-9.55 M. Kasliwal (invited) "Transients in the local Universe: bridging the gap between Novae and Supernovae"

9.55-14.40 Session 1 - SUPERNOVAE: UNDERSTANDING LIGHT CURVES AND SPECTRA

9.55-10.35 R. Kirshner (invited) "Using infrared observations to understand SN Ia"

10.35-11.05 Coffee Break

11.05-11.45 S. Benetti (invited) "20 years of SNIa spectral diversity: what have we learnt?"

11.45-12.05 S. Rodney "HST observations of Type Ia Supernovae at z>1.5"

12.05-12.25 P. Hoeflich "Constraining the Properties of the Progenitors of SNe Ia Using their Light Curves"

12.25-13.45 LUNCH

13.45-14.05 M. Pruzhinskaya "Dust free supernovae Ia and dark energy"

14.05-14.25 V. Stanishev "IFU spectroscopy of host galaxies of SNe Ia"

14.25-16.35 - LEARNING FROM SUPERNOVA REMNANTS

14.25-15.05 K. Long (invited) "Supernova Remnants and their Progenitors"

15.05-15.25 P. Ruiz-Lapuente "Survey for the binary progenitor of SN 1006"

15.25-15.55 Coffee Break

15.55-16.15 W. Kerzendorf "Type Ia progenitor hunt in ancient remnants"

16.15-16.35 A. Chiotellis "The impact of Type Ia progenitor systems on the observational properties of Type Ia supernovae and their remnants"

16.35-16.50 Saurabh Jha “Peculiar Type-Ia Supernovae: Constraining Progenitors and Explosion Models”

Session 2: SYMBIOTIC BINARIES

16.50-17.15 J. Mikolajewska (invited) "Symbiotic stars as possible progenitors of SNIa: System Parameters and Overall Outlook" 17.15-17.40 Jeno Sokoloski (invited) "Symbiotic stars as possible progenitors of SNIa: Accretion and Outflows”

17.40-18.00 S. Mohamed

18-18.20 Mystery object of the day S. Mereghetti "The progenitor of a Ia with a "short delay time"?

18.30 Reception at Caffe’ Pedrocchi: drinks, appetizers, cookies

TUESDAY JULY 5

8.50-10.20 SUPERSOFT X-RAY SOURCES – Moderator: Bob KIrshner

Panelists: M. Gilfanov, M. Kato, R. Di Stefano, M.Orio, M. Nielsen, K. Lepo

M. Gilfanov “Supersoft X-ray Luminosity in External Galaxies”

K. Lepo "Ultra-Soft Sources as Type 1a progenitor candidates"

M. Nielsen "Obscuration of single degenerate type-Ia supernova progenitors in the stellar winds of companion stars."

R. Di Stefano, M. Kato: Comments

10.20-10.50 Coffe Break

10.50-15.30 THE EVOLUTION

10.50-11.30 P. Marigo (invited) "AGB evolution and the initial-final mass relation of single CO WD"

11.30-12.00 E. Garcia-Berro (invited) "The formation and evolution of ONe white dwarfs: prospects for the AIC"

12.00-12.30 C. Tout (invited) "White dwarf remnants of binary stars evolution"

12.30-13.45 LUNCH

13.45-14.05 N. Soker "Double degenerate merging during the common envelope phase"

14.05-14.25 I. Hachisu "A Single Degenerate Progenitor Model of Type Ia Supernovae Highly Exceeding the Chandrasekhar Mass Limit"

14.25-14.45 H. Ge "Stellar Adiabatic Mass-loss model and its applications in common envelope evolution"

14.45-15.05 B. Gaensicke and D. de Martino "Failed SNe Ia"

15.05-15.20 M. R. Schreiber “Evidence for primary mass growth in Cataclysmic Variables”

15.20-15.25 poster presentations

15.25-15.55 Coffee Break

15.55-18.25 CANDIDATE PROGENITORS I - NOVA ERUPTIONS”

15.55-16.35 J. Jose (invited) "Classical and recurrent nova models"

16.35 17.05 M. Kato (invited) “Novae and Accreting WDs as SN Ia Progenitors”

17.05 17.45 R. Williams (invited) "Inferences for CV evolution from spectroscopy"

17.45 -18.15 K. Page (invited) "Swift observations of novae"

20.45 STRINGS CONCERT, UNIVERSITY CONCERT HALL, Piazza Capitaniato

WEDNESDAY JULY 6

8.50-13.30 CANDIDATE PROGENITORS 2 “COMPARISONS, AND THE RECURRENT NOVA PANEL”

8.50-9.30 M. Livio (invited) "On SNe Ia progenitors"

9.30-10.00 M. Henze (invited) “Classical novae as supersoft X-ray sources in the Andromeda galaxy M31”

10.00-10.20 T. Rauch “White Dwarf Model Atmospheres”

10.20-10.50 G.C. Anupama (invited) “Recurrent Novae: What do we know about them?”

10.50-11.20 Coffee Break

11.20-13.30 Recurrent Nova discussion. Moderator: Noam Soker 15 min presentations by S. Starrfield, M. Bode, M. Orio, K. Mukai, D. Buckley

Comprehensive title (see individual abstracts in booklet):

"A new model (Starrfield) – and really new data (high and very high energy, high resolution spectra, the recent recurrent novae): how do they change the scenario?"

13.30-14.30 LUNCH

14.45 Leaving for Verona, Return expected at 19.30

20.45 Mario Livio's public conference

THURSDAY JULY 7

9-12.05 CANDIDATE PROGENITORS 3 – “DOUBLE DEGENERATES AND… OBSERVATIONAL FACTS TO KEEP IN MIND”

9.00-9.40 T. Marsh (invited) "Double White Dwarfs"

9.40-10.15 F. Valsecchi "Tidally-Induced Apsidal Precession in Double White Dwarfs: a new mass measurement tool with LISA" followed by

M. Benacquista & A. Stroeer “Detecting Double progenitors as SNe Ia with LISA” 10.15-10.45 POSTERS PRESENTATIONS

11.10-11.35 M. Kilic "Double White Dwarf Mergers"

11.35-11.55 30 Mystery object of the day: A. Pagnotta "Strong Evidence of a Double-Degenerate Progenitor for One Particular Type Ia Supernova"

12.05-16.20 THE CONSTRAINTS FROM THE OBSERVATIONS

11.55-12.35 F. Patat (invited) "The connection between recurrent novae and some type Ia supernovae"

12.35-13.50 LUNCH

13.50-14.10 A. Sternberg "Evidence for Circumstellar Material in Type Ia Supernovae via Sodium Absorption Features"

14.10-14.30 L. Chomiuk "Constraints on the Progenitors of SNe Type Ia"

14.30-14.50 D. Townsley "Making the Connection: Evaluating How Progenitor Properties Influence Type Ia Supernova Appearance"

14.50-15.10 E. Regos "Progenitor Evolution and Dark Energy Time Variation from CLASH SNe 1a"

15.10-15.30 E.Voss "Observational limits on the SNIa production in stellar clusters"

15.30-15.50 E. Scannapieco "Constraining Models of Type Ia Supernova Progenitors"

15.50-16.10 C. Pritchet "The Delay Time Distribution for Type Ia Supernovae from the SNLS Survey"

16.10-16.40 Coffee Break

16.50 => FRIDAY: EXPLOSION MODELS

16.40 17.20 K. Nomoto "Type Ia supernova models" (invited)

17.20 17.50 F. Roepke (invited) “Thermonuclear supernova explosions from white dwarfs in different progentir systems”

17.50 18.20 S. Sim (invited) "Type Ia supernovae from sub-Chandrasekhar mass white dwarfs"

19.20 Leaving by bus for Conference Dinner on the Colli Euganei

FRIDAY July 8

9 10.30 POPULATION SYNTHESIS ROUND TABLE (part 1)

G. Nelemans (Invited) 25 min (questions during the discussion) “Double White Dwarfs”

N. Mennekens 15 min “Two distributions shedding light on supernova Ia progenitors: delay times and G-dwarf metallicities”

J. Clayes 15 min “Supernovae type Ia and the uncertainties in their progenitor evolution”

M. Moe 15 min “The effects of common envelope and tidal evolution on the rates of SNe Ia”

Discussion 20 min

10.30-11.00 Coffee Break

11 12.30 POPULATION SYNTHESIS ROUND TABLE (part 2)

L. Greggio 15 min

B. Wang 15 min “Helium star donor channel to type Ia supernovae and their surviving companion stars”

L. Piersanti 15 min “He-accreting CO WDs as possible progenitors of Sne Ia”

L. Yungelson 15 min “Type Ia Supernovae and Supersoft X-ray Sources”

Discussion 30 min

13.40 14 Di Stefano

14-15.10 Alternative models F. Forster, R. Pakmor, C. Zhu, J. Guillochon, the titles in order are:

"Hydrostatic carbon burning in carbon oxygen white dwarfs"

"Thermonuclear supernovae from violent mergers of massive CO white dwarfs"

"Properties of CO White Dwarf Merger Remnants"

"Surface Detonations in Double Degenerate Binary Systems Triggered by Accretion Stream Instabilities"

Questions/Discussions at the end

15.10-16 MORE ON MYSTERY OBJECTS

15.10-15.30 Stella Kafka "The changing nature of QU Car: SN Ia progenitor or a hoax?"

15.30-16.00 G. Tovmassian "SDSS0018+3454: a CV, LMXB or Symbiotic Binary?"

16.00-17.15 FINAL DISCUSSION: PLEASE STAY !!!

20 minutes talks by 3 "Mystery Speakers”, in addition to the audience, a panel of “leaders” in each field will ask them some questions

First&name Last&Name Affiliation G.C. Anupama Indian-Institute-of-Astrophysics India Akira Arai Kyoto-Sangyo-University Japan Levon- Aramyan Yerevan-State-University Armenia Christophe Balland LPNHE France Solen Balman Middle-East-Technical-University Turkey Matthew Benacquista Center-for-Gravitational-Wave-Astronomy USA Stefano Benetti INAF-L-OAPd Italy Antonio Bianchini Padova-University Italy David Buckley South-African-Large-Telescope-(SALT) South-Africa Filomena Bufano INAFLOsservatorio-Astronomico-di-Catania Italy Ramon Canal Dept.-of-Astronomy,-University-of-Barcelona Spain Enrico Cappellaro INAF,-Osservatorio-Astronomico-di-Padova Italy Emanuela Chiosi Osservatorio-Astronomico-di-Padova Italy Alexandros Chiotellis Utrecht-University Netherlands-(Greece) Stefano Ciroi Padova-University Italy Laura Chomiuk HarvardLSmithsonian-Cfa/NRAO USA Valentina Cracco Padova-University Italy Joke- Claeys Utrecht-University Netherlands Ashkbiz Danehkar Macquarie-University Australia-(Iran) Domitilla de-Martino INAF-Capodimonte-Astronomical-Obs. Italy Marco De-Pascale INAF-Astronomy-Observatory-of-Padova Italy Massimo Della-Valle INAFLNapoli Italy Rosanne Di-Stefano HarvardLSmithsonian-Center USA Lilia Ferrario Australian-National-University Australia-(Italy) Francisco Forster Universidad-de-Chile Chile Boris Gaensicke University-of-Warwick UK Enrique GarciaLBerro Universitat-Politecnica-de-Catalunya Spain Hongwei Ge Yunnan-Observatory China Diego Gonzalez UNAM-Ensenada,-Mexico Mexico-(Columbia) Laura Greggio INAFLOAPd Italy Marat Gilfanov MPA Germany James Guillochon UC-Santa-Cruz USA Izumi Hachisu University-of-Tokyo Japan Artur Hakobyan Byurakan-Astrophysical-Obs./Yerevan-State-Univ. Armenia Norsiah Hashim University-of-Malaysia Malaysia Diego Hernandez UNAM Mexico Martin Henze Max-Planck-Institute-for-Extraterrestrial-Physics Germany Peter Hoeflich Department-of-Physics USA-(Germany) Narges Jamialahmadi student Iran Saurabh Jha Rutgers-University USA Jordi Jose Universidad-Politecnica-de-Catalunya Spain Stella Kafka NASA/NAI-and-CIW/DTM USA-(Greece) Yasuomi Kamiya University-of-Tokyo-/-IPMU Japan Mansi Kasliwal Caltech USA--(India) Mariko Kato Keio-University Japan Hideyo Kawakita Koyama-Astron.-Obser./Kyoto-Sangyo-University Japan- Edwin Kellogg Harvard/Smithsonian-Cfa USA Wolfgang Kerzendorf Mt-Stromio-Observatory Australia- Mukremin Kilic Smithsonian-Astrophysical-Observatory USA-(Turkey) Robert Kirshner HarvardLSmithsonian-Center USA Oliver Krause Subaru-Telescope,-Nat.Astr.-Obs.of-Japan Japan Laurits Leedjarv Tartu-Observatory Estonia Bruno Leibundgut ESO Germany Kelly Lepo University-of-Toronto Canada Vladimir Lipunov Sternberg-Astronomical-Ins.,-Moscow-State-Univ. Russia Mario- Livio Space-telescope-Science-Institute-(STScI) USA-(Israel) Knox Long STScI USA Paola Marigo University-of-Padova,-Astronomy-Department Italy Thomas- Marsh University-of-Warwick UK Michael Maxwell University-of-Central-Lancashire UK Curtis McCully Rutgers,-The-State-University-of-New-Jersey USA Nicki Mennekens Vrije-Univ. Belgium Sandro Mereghetti INAF-IASF-Milano Italy Joanna Mikolajewska N.-Copernicus-Astronomical-Center Poland Max Moe Harvard-University USA- Shazrene Mohamed University-of-Bonn Germany-(Zimbabwe) Martine- Mouchet APC France Koji Mukai NASA/GSFC/CRESST-and-UMBC USA-(Japan) Ulisse Munari INAF-Astronomy-Observatory-of-Padova Italy Masayoshi Nagashima Kyoto-Sangyo-University Japan- Gijs Nelemans Raboud-University-Nijmegen Netherlands Mikkel Nielsen Radboud-University-Nijmegen Netherlands Ken'ichi Nomoto IPMU/University-of-Tokyo Japan- Jun Okumura Kyoto-University Japan-(India) Marina Orio INAFLPadova-and-Univ.-of-Wisconsin Italy,-USA Magdalena Otulakowska N.-Copernicus-Astronomical-Center Poland Rachid Ouyed University-of-Calgary Canada Kim Page University-of-Leicester UK Ashley Pagnotta Lousiana-State-University USA Nando Patat ESO Germany-(Italy) Yakup Pekon Middle-East-Technical-University Turkey Gohar Yerevan-State-University Armenia Luciano Piersanti INAFLOATe Italy Onno Pols Astronomical-Institute,-Utrecht-University Netherlands Dina Prialnik Tel-Aviv-University Israel Chris Pritchet University-of-Victoria Canada Maria Pruzhinskaya Sternberg-Astronomical-Ins.,-Moscow-State-Univ. Russia Maria-Letizia Pumo INAF-L-OAPd Italy Thomas Rauch Eberhard-Karls-Univ. Germany Eniko Regos ELTE/CERN Switzerland Alvio Renzini INAF Italy Valerio Ribeiro Astrophysics,-Cosmology-&-Gravity-Center UK-(Mozambique) Steven Rodney The-Johns-Hopkins-University USA Friedrich Roepcke max-Planck-for-Astrophysics,-Garching Germany Pilar RuizLLapuente University-of-Barcelona Spain Mark Rushton Jeremiah-Horrocks-Institute UK Tenay Saguner Universita-degli-Studi-di-Padova Italy Dave Sahman Sheffield-University UK A.-Talat Saygac Istanbul-University,-Faculty-of-Science Turkey Evan Scannapieco Arizona-State-University USA Linda Schmidtobreick European-Southern-Observatory Chile Matthias-R. Schreiber Univ.-of-Valparaiso,-Dept.-Physics-and-Astronomy Chile Sergey Shugarov Sternberg-Astronomy-Institute Russia Stuart Sim RSAA,-ANU Australia Jonathan- Smoker European-Southern-Observatory Chile Noam Soker Technion israel Jennifer-(Jeno)Sokoloski Columbia-University USA Sumner Starrfield Arizona-State-University USA Assaf Sternberg Weizmann-Institute-of-Science Israel Nao Suzuki Lawrence-Berkeley-National-Lab USA Anna Tatarnikova Sterberg-Astronomical-Institute Russia Silvia Toonen IMAPP,-Radbound-Univ.-Nijmegen Netherlands Luis Torres Instituto-de-Astronomia-L-UNAM Mexico-(Columbia) Christopher Tout University-of-Cambridge UK Gagik Tovmassian UNAM,-Ensenada Mexico-(Armenia,-USA) Dean Townsley University-of-Alabama USA Takuji Tsujimoto National-Astronomical-Observatory-of-Japan Japan Massimo Turatto INAF-Osservatorio-di-Trieste Italy Francesca Valsecchi CIERA-and-Northwestern-University USA Irina Voloshina Sternberg-Astronomical-Institute Russia Rasmus Voss Radboud-University-Nijmegen Netherlands Bo Wang Yunnan-Observatory,Chinese-Academy-of-Sciences China Ronald Webbink University-of-Illinois USA Dayal Wickramasinghe Australian-National-University Australia Robert Williams STScI USA Masayuki Yamanaka Hiroshima-University Japan Lev Yungelson Institute-of-Astronomy Rusia Luca Zampieri INAFLAstronomical-Observatory-of-Padova Italy Polina Zemko -Moscow-State-University Russia Chenchong Zhu University-of-Toronto Canada IAU Symposium 281 Binary Paths to type Ia Supernovae Explosions

Three months after the end of this symposium, the Nobel prize for physics was awarded to three astrophysicists who inferred the existence of dark energy from type Ia supernovae data. Undoubtedly, it was a great year for scientists working on the mystery represented by type Ia supernovae. The environment of the IAU Symposium 281 resonated with energy and enthusiasm, the sessions were exciting and full of ideas. Although the number that gathered at Padova in July of 2011 was smaller than in other, more general symposia, we are proud to say that we organized the meeting of a vibrating, very active group of scientists. 131 participants came from 30 different countries. A third were women, reflecting well the present composition of the world’s astronomers’ population. We had made an experiment, constituting a Scientific Organizing Committee of 16 women and one man. This did not attract a larger women to participate than the actual fraction of women working in our field, however we believe it was a positive experience, creating a feeling of a gender-bias-free atmosphere and facilitating young women’s participation in the discussions. It was also a small provocative action to make our colleagues talk about gender biases in astronomy, and we think it worked positively. Graduate students and young post-doctoral were a large fraction and the attendees. The many young participants brought enthusiasm and new ideas. The atmosphere was thus refreshing, charged with expectations and possibilities. I have only one regret: since we had to announce the symposium dates a year and a half in advance, thereby missing the possibility to adjust the dates depending on new proposed conference of related subjects. A large supernova conference was held in Australia shortly before our symposium on the progenitors, so potential US participants found it difficult to travel to two different continents within a fortnight. However, the participation of the supernova scientists, theorists and observers alike, was fundamental for the success of the symposium, meant to bring together different communities of astrophysicists: those working on supernovae, on close binary evolution, and on binary populations. A previous “SNova” semester- long program and conference were held 5 years earlier at the Kavli Institute in Santa Barbara. Those of us who took part either of them came home enriched and energized. Our aim was to rekindle the spirit of this previous experience and I am proud to say we were successful. There were many highlights in this conference and by mentioning a few I do not want to downplay the importance of any of the other topics. As a ``nova’’ scientist, I found it fascinating to learn about the variety of possible models leading to the explosion and the possibility of ``sub-Chandra’’ models seems to be intriguing and important to explore. A short talk by S. Mohamed on detailed simulations of the Roche lobe overflow seemed innovative and sparked many questions and discussions. The possibility of detecting gravitational waves from close binaries with white dwarfs with LISA in future years is very exciting. The population synthesis calculations in the new era of large surveys with unprecedented statistics are more important than ever. The unexpected bonus of three eruptions of luminous recurrent novae within a little over two years before this Symposium, allowed new estimates of WD masses and compositions. The possibility that many recurrent novae may host neon oxygen white dwarfs seems less unlikely now. Brand new spectra of the 10m South African large Telescope were presented almost in ``real time’’. Optical spectroscopy appears also to be fundamental in probing the environment in which SNe Ia explode, and Patat’s talk on the likely ``recurrent-nova- like’’ circumstellar environment opened up new possibilities to search for the signature of single degenerate progenitors. Kilic’s radial velocity studies are paving a new avenue to search for double degenerates and obtain statistics of these systems. Marat Gilfanov was invited to take part in a debate with several of us to defend his position that the integrated supersoft X-ray luminosity of galaxies may rule out a large contribution of single degenerate progenitors. Many of us had a different opinion, so we confronted results and theoretical predictions. To me, this all science is about, constantly testing one’s results and confronting them with others. I am proud to say we achieved this goal in Padova. Throughout the Symposium we experienced that tense and vibrating atmosphere that fosters intellectual and scientific development. For me, the best part of the conference was the participation of three very young scientists from developing countries, at the initial stages of graduate studies, who obtained a grant to participate not only in the Padova conference, but also doing research in Italy for the whole Summer. Levon Aramayan from Armenia, Narges Jami-Aliahamadi from Iran and Norsia Hashim from Malaysia were a wonderful presence with their fresh ideas and enthusiasm. Spending the Summer in contact with them and following their first steps in scientific research was very rewarding and made even the days of the Symposium more meaningful for me. Many thanks to the ``mystery speakers’’ selected without knowledge of the other particpants to summarize the symposium at the end. Mukremin Kilic, Lilia Ferrario and Alvio Renzini did an excellent job focusing on ``what we were taking home’’ from this conference. Special thanks go to the participants who gave public talks to the general public in Padova: Mario Livio, Lilia Ferrario and Bob Williams. Their contribution was greatly appreciated by a large number of people in the community in which we live! Finally, we offered an interesting and entertaining social program, with nice welcome parties and a wonderful dinner on the Colli Euganei. However, the restrictions on the registration fee and the greatly increased publication cost of the proceedings posed some challenges and made the finances difficult to manage for a small symposium. For instance, the majority of the scientififc committee thought that a common venue for the lunches was important to keep up the discussions and to save time in the middle of the day, but unfortunately we could not offer a discount price and guarantee the restaurant a minimum number of participants because there was no way to include lunch in the registration fee budget. I will not dwell here on other finance-related problems, but I would like to let the IAU know that more flexibility on the registration fee would actually make the total cost to the participants smaller, not larger. This is especially important for the smaller, more specifically focused symposia, which I believe are also very important to bring forward the scientific mission of the IAU.

IAU POST MEETING REPORT FORM

1. Meeting Number: IAU Symposium 282

2. Meeting Title: “From Interacting Binaries to Exoplanets: Essential Modeling Tools”

http://www.astro.sk/IB2E/

3. Coordinating Division: Division V Variable Stars Supporting Divisions: Division III Planetary Systems Sciences Division IV Stars Division IX Optical & IR Techniques

Supporting Commissions: C25 Stellar Photometry & Polarimetry C27 Variable Stars C29 Stellar Spectra C36 Theory of Stellar Atmospheres C42 Close Binary Stars C53 Extrasolar Planets (WGESP) C54 Optical & Infrared Interferometry

4. Dedication of meeting: ! This! meeting! commemorated! the! 40th! anniversary! of! the! first! model! atmosphere! and! binary! star! synthesis! codes,! as! well! as! the! 110th! anniversary! of! the birth of Dr. Antonín Bečvář, founder of the Skalnate Pleso Observatory and author of several famous atlases and catalogues: Atlas Coeli, Atlas Borealis, Atlas Eclipticalis and Atlas Australis! which! were! used!nightly!by!astronomers!around!the!world!for!almost!half!a!century.

5. Location (city, country): Tatranska Lomnica, Slovak Republic

6. Dates of meeting: July 18 - 22, 2011

7. Number of participants: 207 registered for the meeting (194 astronomers, 13 others); 189 attended the meeting (177 astronomers, 12 others)

8. List of represented countries: 31 countries Australia, Austria, Bulgaria, Canada, Chile, Croatia, Czech Republic, Finland, France, Germany, Greece, Hungary, Iran, Israel, Italy, Japan, Korea, Latvia, Netherlands, New Zealand, Poland, Portugal, Russia, Serbia and Montenegro, Slovak Republic, Spain, Switzerland, Turkey, Ukraine, United Kingdom, United States

9. Report submitted by: Mercedes Richards and Ivan Hubeny, SOC Chairs

10. Date and place: August 5, 2011 in Tatranska Lomnica, Slovakia

11. Signature of SOC Chairperson:

IAUS 282: From Interacting Binaries to Exoplanets: Essential Modeling Tools

SOC: Scientific Organizing Committee Mercedes Richards, chair (USA) Ivan Hubený, co-chair (USA) Dmitry Bisikalo (Russia) Ján Budaj (Slovakia) Osman Demircan (Turkey) Gojko Djurasevic (Serbia) Edward Guinan (USA) Petr Hadrava (Czech Republic) Petr Harmanec (Czech Republic) Ladislav Hric (Slovakia) Pavel Koubský (Czech Republic) Panagiotis Niarchos (Greece) Geraldine (USA) Theodor Pribulla (Slovakia) Didier Queloz (Switzerland) Philippe Stee (France) Paula Szkody (USA) Juraj Zverko (Slovakia) Simon Portegies Zwart (Netherlands) ! ! LOC: Local Organizing Committee Theodor Pribulla, chair Ladislav Hric, co-chair Anna Bobulová Ján Budaj Zuzana Cariková Drahomír Chochol Ľubomír Hambálek Richard Komžík Emil Kundra Matej Sekeráš Augustín Skopal Martin Vaňko Juraj Zverko

IAUS 282: From Interacting Binaries to Exoplanets: Essential Modeling Tools

Astronomical Institute, Slovakia, July 17 – 22, 2011

Sunday July 17, 2011 13:00 – 18:00 Registration 18:00 Welcome Party/Cocktails (at the conference hotel Academia)

Monday July 18, 2011 7:30 – 10:00 Registration

Opening Ceremony Chair: Trimble 8:30 Aleš Kucera Welcome by Institute Director 8:40 T. Pribulla/L. Hric Welcome by LOC Chairs 8:45 M. Richards/ I. Hubeny Welcome by SOC Chairs 8:50 Petr Harmanec Shaking the Pot of Modeling Tools: Some Open Problems in the Field

Session A: Multiwavelength Photometry and Spectroscopy of Interacting Binaries Chair: Karen Bjorkman 9:05 Edward Guinan Advances in Telescope and Detector Technology - Impacts on the Study and Understanding of and Exoplanet Systems 9:40 Panagiotis Niarchos Ground-based and Space Observations of Interacting Binaries 10:05 Alceste Bonanos Techniques for Observing Binaries in Other Galaxies 10:30 Coffee Break and Mini Talks: A01–A35 (11 talks, Chair: Mercedes Richards) 11:35 Laurent Eyer The Impact of Gaia and LSST 12:10 Carla Maceroni The Impact of CoRoT and Kepler 12:35 Geraldine Peters Use of the Virtual Observatory Databases in Binary Star Research 13:00 Lunch

Session B: Observations and Analysis of Exoplanets and Brown Dwarfs Chair: Wilhelm Kley 14:30 Didier Queloz Exoplanets from the Techniques and Analysis Tools Perspective 15:05 Thomas Pasternacki Homogeneous Study of the Light Curves of CoRoT Exoplanets 15:30 Styliani Kafka Challenges to Observations of Low Mass Binaries 16:05 Coffee Break and Mini Talks: B01—B15, C01—C10 (8 talks, Chair: Ivan Hubeny) 17:10 Katelyn Allers Brown Dwarfs in Binaries 17:35 Maciej Konacki Detecting and Characterizing Exoplanets in Binary Star Systems 18:00 Panel Discussion Sessions A, B

Tuesday July 19, 2011 Session C: Imaging Techniques for Binary Stars, Brown Dwarfs, and Exoplanets Chair: Theodor Pribulla 9:00 Philippe Stee Binaries and Multiple Systems Observed with the VLTI, NPOI and CHARA/VEGA Interferometric Eyes 9:35 Eugene Serabyn Observing Close to Bright Stars Using Vortex Coronagraphy, Visible- Wavelength Adaptive Optics, and Nulling Interferometry 10:00 Mercedes Richards Tomography of Interacting Binaries 10:25 Coffee Break 10:45 Karen Bjorkman Polarimetry of Close Binaries and Exoplanets 11:20 Sasha Hinkley Adaptive Optics Imaging of Binaries, Brown Dwarfs, and Exoplanets: Present and Future 11:55 Tobias Schmidt Direct Observations of Sub-Stellar Companions Around Young Stars 12:20 Break 12:30 Official Excursion

Wednesday July 20, 2011 Session D: Model Atmospheres of Stars, Interacting Binaries, Disks, Exoplanets, and Brown Dwarfs Chair: Orsola De Marco 9:00 Piercarlo Bonifacio Calculation of LTE Atmospheres with ATLAS, MARCS and CO5BOLD 9:25 Ivan Hubeny Basic Tools for Modeling Stellar and Planetary Atmospheres 10:00 John Hillier Hot Stars with Winds: The CMFGEN Code 10:25 Coffee Break and Mini Talks: D01—D11 (6 talks, Chair: Robert Wilson) 11:30 France Allard Stellar to Substellar Atmosphere 2-3D RHD Simulations with Cloud Formation and Rotation using CO5BOLD and PHOENIX 12:05 Hilding Nielson Comparison of Limb-Darkening Laws from Plane-Parallel and Spherical ATLAS Model Atmospheres 12:30 Tomislav Jurkic Modelling of Dust Around the Symbiotic Nova RR Tel 12:55 Lunch

Session E: Synthetic Light Curves, Velocity Curves, Spectra of Binary Stars, and Spectra of Binaries with Accretion Structures Chair: Philippe Stee 14:30 Andrej Prsa Advances in Modeling Eclipsing Binary Stars in the Era of Large All- Sky Surveys with EBAI and PHOEBE 15:05 Theodor Pribulla ROCHE: Analysis of Eclipsing Binary Multi-Dataset Observables 15:30 Albert Linnell The BINSYN Program 15:55 Coffee Break and Mini Talks: E01—E24 (12 talks, Chair: Geraldine Peters) 17:00 Stefan Mochnacki Application of the GDDSYN Method in the Era of KEPLER, CoRoT, MOST and BRITE 17:25 Ján Budaj Synthetic Spectra and Light Curves of Interacting Binaries and Exoplanets with Circumstellar Material: SHELLSPEC 18:00 Panel Discussion Sessions C, D, E

Thursday July 21, 2011 Session F: Techniques for Analysis of Spectra and Light Curves Chair: France Allard 9:00 Petr Hadrava The Disentangling of Stellar Spectra 9:35 Kresimir Pavlovski Quantitative Spectroscopy of Binary Stars 10:00 Slavek Rucinski Spectral Analysis: The Broadening Function Technique 10:25 Coffee Break and Mini Talks: F01—F07, G01—G13 (10 talks, Chair: Edward Devinney) 11:15 Shay Zucker TODCOR - A Two Dimensional Correlation Technique 11:50 Simon Albrecht The Long History of the Rossiter-McLaughlin Effect and its Recent Applications 12:15 Amaury Triaud The Rossiter McLaughlin Effect on Transiting Planets and Low Mass Eclipsing Binaries 12:40 Zdenek Mikulasek Period Analyses Without O-C Diagrams 13:05 Lunch

Session G: Formation and Evolution of Binary Stars, Brown Dwarfs, and Planets Chair: Peter Eggleton 14:30 Cathie Clarke The Formation of Binary stars 15:05 Christopher Tout Non-conservative Evolution of Binaries with STARS 15:40 Satoshi Mayama Direct Imaging of Bridged Twin Protoplanetary Disks in a Young Multiple Star 16:05 Coffee Break and Mini Talks: G14—G30 (8 talks, Chair: Dmitry Bisikalo) 16:55 Wilhelm Kley Formation and Evolution of Exoplanets 17:30 Adam Burrows Towards a Theory for the Atmospheres, Structure, and Evolution of Giant Exoplanets 18:05 Panel Discussion Sessions F, G

19:30 Conference Reception

Friday July 22, 2011 Session H: Hydrodynamic Simulations of Exoplanets and Mass Transfer in Interacting Binaries Chair: Adam Burrows 9:00 Dmitry Bisikalo Gas Dynamic Simulations of Mass Transfer in Cataclysmic Variables 9:35 Orsola De Marco Hydrodynamic Simulations of the Common Envelope Binary Interaction 10:00 Tatiana Demidova Hydrodynamics of Young Binaries with the Low-mass Secondary 10:25 Coffee Break and Mini Talks: H01—H04!(3!talks,!Chair:!Mercedes!Richards) 11:15 Helmut Lammer Simulations of Exoplanetary Atmosphere Environments 11:50 Ian Dobbs-Dixon 3D Models of Exoplanet Atmospheres 12:15 Elke Pilat-Lohinger Dynamical Stability and Habitability of Extrasolar Planets 12:40 Panel Discussion Session H 13:00 Lunch

Closing Ceremony Chair: Alan Batten 14:30 Pavel Koubsky Summary of Observational Techniques 14:50 Adam Burrows Summary of Theoretical Techniques 15:10 Theodor Pribulla LOC Closing Remarks 15:20 Mercedes Richards SOC Closing Remarks

17:00 Education and Public Outreach Event in Poprad (in Czech language) Ivan Hubeny Hledani!a!studium!planet!mimo!Slunecni!soustavu! ! ! ! ! Detecting!and!Studying!Exoplanets

Saturday July 23, 2011 9:00 Tour of Skalnate Pleso Observatory

IAU Symposium 282: List of Participants

Delegate Name Organisation Dr. Simon Albrecht Massachusetts Institute of Technology, Kavli Institute for Astrophysics and Space Research, USA Ms. Julia Alfonso-Garzon Centro de Astrobiologia (INTA-CSIC), Spain Dr. France Allard Centre de Recherche Astrophysique de Lyon, Ecole Normale Superieure de Lyon, France Prof. Katelyn Allers Bucknell University, USA Dr. Roman Baluev Central (Pulkovo) Astronomical Observatory of Russian Academy of Sciences, Russia Ms. Daniela Barria Universidad de Concepcion-ESO, Chile Prof. Alan Batten National Research Council Canada, Canada Ms. Carolina Bergfors Max-Planck-Institute for Astronomy, Germany Prof. Dmitry Bisikalo Institute of astronomy of Russian Academy of Science, Russia Prof. Jon Bjorkman Dept. of Physics and Astronomy, University of Toledo, USA Prof. Karen Bjorkman Dept. of Physics and Astronomy, University of Toledo, USA Prof. Nikolai Bochkarev Sternberg Astronomical Institute at Lomonosov Moscow State University, Russia Dr. Alceste Bonanos IAA, National Observatory of Athens, Greece Dr. Mariangela Bonavita Department of Astronomy and Astrophysics, , Canada Dr. Piercarlo Bonifacio GEPI, Observatoire de Paris, CNRS, Univ Paris Diderot, France Dr. Jan Budaj Astronomical Institute, Tatranska Lomnica, Slovakia Dr. Edwin Budding Carter Observatory and Dept. of Physics & Astronomy, University of Canterbury, New Zealand Prof. Adam Burrows Department of Astrophysical Sciences, Princeton University, USA Ms. Zuzana Carikova Astronomical Institute, Slovak Academy of Sciences, Slovakia Ms. Lale Celik Ankara University, Faculty of Science, Astronomy and Space Sciences Department, Turkey Dr. Carlson Chambliss Kutztown University, USA Dr. Drahomir Chochol Astronomical Institute of the Slovak Academy of Sciences, Slovakia Mr. Marek Chrastina Department of Theoretical Physics and Astrophysics, Masaryk University, Brno, Czech Republic Dr. Eleftheria Christopoulou Department Of Physics, University of Patras, Greece Prof. Cathie Clarke Institute of Astronomy, University of Cambridge, UK Mr. Attila Cseki Astronomical Observatory of Belgrade, Serbia and Montenegro Dr Szilard Csizmadia German Aerospace Center, Institute for Planetary Research, Germany Mr. Sebastian Daemgen ESO Garching, Germany Mr. Ashkbiz Danehkar Macquarie University, Australia Dr. Avril Day-Jones Universidad de Chile, Chile Prof. Orsola De Marco Macquarie University, Australia Dr. Tatiana Demidova Pulkovo Observatory of Russian Academy of Sciences, Russia Prof. Osman Demircan Canakkale Onsekiz Mart University, Department of Physics, Canakkale, Turkey Prof. Edward Devinney, Jr. Department of Astronomy & Astrophysics, Villanova University, USA Dr. Gojko Djurasevic Astronomical Observatory of Belgrade, Serbia and Montenegro Dr. Ian Dobbs-Dixon University of Washington, USA Mgr. Marek Drozdz Mt. Suhora Astronomical Observatory, Krakow (Cracow) Pedagogical University, Poland Dr. Peter Eggleton Lawrence Livermore National Laboratory, USA Dr Laurent Eyer Observatoire de Geneve, Switzerland Dr. Juris Freimanis Ventspils International Radio Astronomy Centre, Ventspils University College, Latvia Dr. Barbara Funk Institut for Astronomy, University of Vienna, Austria Dr. Rudolf Galis P. J. Safarik University, Slovakia Dr. Kosmas Gazeas - ESTEC, Netherlands Ms. Joana Gomes University of Hertfordshire, UK Dr. Jonay Gonzalez Hernandez Instituto de Astrofisica de Canarias, Spain Dr. Jose Groh Max-Planck Institute for Radioastronomy, Germany Dr. Jiri Grygar Institute of Physics, Czech Academy of Sciences, Prague, Czech Republic Prof. Edward Guinan Astronomy & Astrophysics, Villanova University, USA Prof. Petr Hadrava Astronomical Institute of the Academy of Sciences of the Czech Republic Ms. Kelly Hambleton Jeremiah Horrochs Institute, University of Central Lancashire, UK Prof. Dr. Petr Harmanec Astronomical Institute of the Charles University of Prague, Czech Republic Dr. Artie Hatzes Thueringer Landessternwarte Tautenburg, Germany Dr. Tibor Hegedus Baja Astronomical Observatory, Hungary Prof. D. John Hillier University of Pittsburgh, USA Dr. Sasha Hinkley California Institute of Technology, USA Dr. Ladislav Hric Astronomical Institute, Slovak Academy of Sciences, Slovakia Dr. Ivan Hubeny University of Arizona, USA Prof. Dr. Ilian Iliev Institute of Astronomy and Rozhen National Astronomical Observatory, Bulgarian Academy of Sciences Dr. Lubomir Iliev Institute of Astronomy and Rozhen National Astronomical Observatory, Bulgarian Academy of Sciences Dr. Gulay Inlek Physics Department, Balikesir University, Turkey none Dmitry Ionov Institute of Astronomy of the Russian Academy of Sciences, Russia Dr. Jan Janik Departament of Theoretical Physics and Astrophysics, Masaryk University, Brno, Czech Republic Mr. Tomislav Jurkic Department of Phyisics, University of Rijeka, Rijeka, Croatia Ms. Monika Jurkovic Astronomical Observatory of Belgrade, Serbia and Montenegro Dr. Zsolt Kovari Konkoly Observatory, Hungary Dr. Stella Kafka NASA Astrobiology Institute and Carnegie Institution of Washington/DTM, USA Dr. Belinda Kalomeni University of Ege, Department of Astronomy & Space Sciences, 35100 Izmir-Turkey Dr. Young-Woon Kang Sejong University, Korea Dr. Eugenia Karitskaya Institute of Astronomy of RAS, Russia Dr. Laszlo Kiss Konkoly Observatory, Hungary Prof. Wilhelm Kley Institute for Astronomy & Astrophysics, University of Tuebingen, Germany Ing. Vladimir Kolbas Department of Physics, University of Zagreb, Croatia Dr. Maciej Konacki NCAC Polish Academy of Sciences, Poland Mr. Piotr Konorski Astronomical Observatory, University of Warsaw, Warsaw, Poland Dr. Daniela Korcakova Astronomical Institute, Charles University, Czech Republic Prof. Dubravka Kotnik-Karuza Department of Physics, University of Rijeka, Croatia Dr. Pavel Koubsky Astronomicky Ustav AV CR, v.v.i, Observatory Ondrejov, Czech Republic Ms. Evgenia Koumpia National Observatory of Athens, Greece Prof. Jerzy Kreiner Mt. Suhora Observatory, Cracow Pedagogical University, Poland Ms. Tereza Krejcova Department of Theoretical Physics and Astrophysics, Masaryk University, Brno, Czech Republic Dr. Emil Kundra Astronomical Institute, Slovak Academy of Sciences, Slovakia Mgr. Petr Kurfurst Department of Theoretical Physics and Astrophysics, Masaryk University, Brno, Czech Republic Prof. Diana Kyurkchieva Shumen University, Bulgaria Dr. Helmut Lammer Austrian Academy of Sciences, Space Research Institute, Austria Ms. Olivera Latkovic Astronomical Observatory of Belgrade, Serbia and Montenegro Dr. Jae Woo Lee Korean Astronomy and Space Science Institute, Korea Dr. Chung-Uk Lee Korean Astronomy and Space Science Institute, Korea Dr. Holger Lehmann Thueringer Landessternwarte Tautenburg, Germany Ms. Jiri Liska Dept. of Theoretical Physics & Astrophysics, Masaryk University, Czech Republic Mr. Alexios Liakos Dept. Astrophysics, Astronomy and Mechanics, National and Kapodistrian University of Athens, Greece Dr. Albert Linnell Astronomy Department, University of Washington, USA Dr. Steven Macenka Jet Propulsion Laboratory, USA Dr. Carla Maceroni INAF- Osservatorio Astronomico di Roma, Italy Dr. Dragomir Marchev Shumen University, Bulgaria Mr. Konstantinos Markakis National Observatory of Athens, I. Metaxa & Vas. Pavlou St., P. Penteli 15236, Greece Dr. Satoshi Mayama The Graduate University for Advanced Studies, Kanagawa, Japan Dr. Ronald Mennickent Departamento de Astronomia, Universidad de Concepcion, Chile Mr. Peter Miklos Institute of Physics, Faculty of Natural Sciences, University of P.J.Safarik, Slovakia Prof. Zdenek Mikulasek Department of Theoretical Physics and Astrophysics, Masaryk University, Brno, Czech Republic Mr. Ivan Milic Astronomical Observatory of Belgrade, Serbia and Montenegro Dr. David Mkrtichian Crimean Astrophysical Observatory, Ukraine Dr. Stefan Mochnacki Dept. of Astronomy and Astrophysics, University of Toronto, Canada Dr. Michele Montgomery University of Central Florida, USA Dr. Helena Morais Department of Physics, I3N, University of Aveiro, Portugal Mr. Jozef Nedoroscik Institute of Physics, Faculty of Natural Sciences, University of P. J. Safarik, Slovakia Dr. Hilding Neilson Argelander Institute for Astronomy, University of Bonn, Germany Ms. Jana Nemravova Astronomical Institute, Faculty of Mathematics and Physics, Charles University, Czech Republic Dr. Vitaly Neustroev University of Oulu, Finland Prof. Panagiotis Niarchos Dept. Astrophysics, Astronomy and Mechanics, National and Kapodistrian Unversity of Athens, Greece Dr. Nikolay Nikolov Max Planck Institute for Astronomy, Germany Dr. Waldemar Ogloza Cracow Pedagogical University, Poland Dr. Katalin Olah Konkoly Observatory of the Hungarian Academy of Sciences, Hungary Ms. Magdalena Otulakowska-Hypka N. Copernicus Astronomical Center of the Polish Academy of Sciences, Poland Mr. Thomas Pasternacki German Aerospace Center (DLR), Institute of Planetary Research, Germany Dr. Ernst Paunzen Institute for Astronomy, University of Vienna, Austria Prof. Kresimir Pavlovski Department of Physics, University of Zagreb, Croatia Prof. Geraldine Peters University of Southern California, USA Dr. Elke Pilat-Lohinger Institute of Astronomy, University of Vienna, Austria Dr. Bogumil Pilecki Warsaw University Observatory, Warszawa, Poland Mr. Antonio Pilello Georg-August-Universitat Gottingen, Institut fur Astrophysik, Germany Mgr. Eva Plavalova Comenius University in Bratislava, Faculty of Mathematics, Physics and Informatics, Slovakia Ms. Elena Popova Pulkovo Observatory of Russian Academy of Sciences, Russia Dr. Theodor Pribulla Astronomical Institute of the Slovak Academy of Sciences, Slovakia Dr. Andrej Prsa Villanova University, USA Prof. Didier Queloz University of Geneva, Observatoire de Geneva, Switzerland Ms. Milena Ratajczak NCAC Polish Academy of Sciences, Poland Dr. Phillip Reed Kutztown University of Pennsylvania, USA Mgr. Valeria Reckova Hvezdaren a Planetarium, Hlohovec, Slovakia Prof. Mercedes Richards Pennsylvania State University, USA Prof. Slavek Rucinski Department of Astronomy and Astrophysics, University of Toronto, Canada Dr. Domagoj Ruzdjak Hvar Observatory, Faculty of Geodesy, Croatia Ms. Mariza Sarta Dekovic Department of Physics, University of Rijeka, Croatia Dr. Tobias Schmidt Astrophysikalisches Institut und Universitats-Sternwarte Jena, Germany Dr. Richard Schwarz Institut efor Astronomy, University of Vienna, Austria Ms. Klara Sejnova Department of Theoretical Physics and Astrophysics, Masaryk University, Brno, Czech Republic Mgr. Matej Sekeras Astronomical Institute of the Slovak Academy of Sciences, Slovakia Dr. Hakan Senavci Ankara University, Astronomy and Space Sciences Department, Tandogan, Ankara, Turkey Dr. Eugene Serabyn Jet Propulsion Laboratory, USA Ms. Brigitta Sipocz Centre for Astrophysics Research, University of Hertfordshire, UK Dr. Petr Skoda Astronomical Institute of the Academy of Sciences of the Czech Republic Dr. Augustin Skopal Astronomical Institute, Slovak Academy of Sciences, Tatranska Lomnica, Slovakia Dr. Greg Stachowski Mt. Suhora Astronomical Observatory, Poland Dr. Ivanka Stateva Institute of Astronomy and Rozhen National Astronomical Observatory, Academy of Sciences, Bulgaria Dr. Philippe Stee Observatoire de la Cote d'Azur - CNRS - Universite de Nice Sophia Antipolis, France Dr. Guy Stringfellow Center for Astrophysics and Space Astronomy, University of Colorado, USA Dr. Davor Sudar Hvar Observatory, Faculty of Geodesy, Zagreb, Croatia Dr. Gyula Szabo MTA Konkoly Observatory, Hungary Mr. Tamas Szalai Department of Optics and Quantum Electronics, University of Szeged, Hungary Dr. John Southworth/Taylor Keele University, UK Prof. Christopher Tout University of Cambridge, UK Dr. Amaury Triaud Observatoire de l'Universite de Geneve, Switzerland Prof. Virginia Trimble University of California, USA Dr. Martin Vanko Astronomical Institute, Slovak Academy of Sciences, Slovakia Ms. Aline Vidotto University of St Andrews, UK Dr. Istvan Vince Astronomical Observatory of Belgrade, Serbia and Montenegro Ms. Carolina von Essen Hamburger Sternwarte, Germany Dr. Viktor Votruba Stellar Department, Astronomical Institute, Academy of Sciences of the Czech Republic Ms. Gemma Whittaker , UK Prof. Robert Wilson University of Florida, Gainesville, USA Dr. Marek Wolf Astronomical Institute, Faculty of Mathematics and Physics, Charles University, Czech Republic Dr. Taras Yakobchuk Main Astronomical Observatory of the National Academy of Sciences, Ukraine Dr. Kadri Yakut University of Ege, Turkey Ms. Olga Zakhozhay Main Astronomical Observatory, National Academy of Sciences, Ukraine Mr. Bartlomiej Zakrzewski Mt. Suhora Observatory, Cracow Pedagogical University, Poland Dr. Petr Zasche Astronomical Institute, Faculty of Mathematics and Physics, Charles University Prague, Czech Republic Dr. Miloslav Zejda Department of Theoretical Physics and Astrophysics, Masaryk University, Brno, Czech Republic Mgr. Pawel Zielinski Torun Centre for Astronomy of the Nicolaus Copernicus University, Poland Dr. Jozef Ziznovsky Astronomical Institute, Slovak Academy of Sciences, Tatranska Lomnica, Slovak Republic Prof. Staszek Zola Astronomical Observatory, Jagiellonian University, Poland Prof. Shay Zucker Tel Aviv University, Israel Dr. Juraj Zverko Astronomical Institute, Slovak Academy of Sciences, Slovakia

Accompanying Astronomers Mr. Arkadiusz Hypki N. Copernicus Astronomical Center of the Polish Academy of Sciences Ms. Eun-Jeong Kim Korea Astronomy and Space Science Institute Ms. Jeong Eun Lee Korea Astronomy and Space Science Institute Dr. Martin Netopil University of Vienna DR. Monika Rode-Paunzen Institute for Astronomy, University Vienna Ms. Tatiana Tsvetkova Institute of Astronomy Russian Academy of Sciences

Scientific Highlights of IAU Symposium 282

From Interacting Binaries to Exoplanets: Essential Modeling Tools

IAU Symposium 282 entitled “From Interacting Binaries to Exoplanets: Essential Modeling Tools” was organized to bring the exoplanet and binary star communities together to discuss the many techniques that are already being shared, and that may possibly be shared in the future. More specifically, the goal was to demonstrate the extent to which current computer programs are effective in modeling observations of interacting binary stars, brown dwarfs, and exoplanets; to identify ways to improve these codes by incorporating more detailed and realistic physics, while maximizing computer capacity; and to examine how to utilize active and proposed survey projects like Kepler, LSST, and Gaia to obtain data of the highest quality that can be modeled to extract optimal physical parameters, specifically to improve our understanding of the physics. The acceleration of discoveries of brown dwarfs and exoplanets and the rapid influx of very precise light curves from programs like CoRoT and Kepler provide additional stimuli for improving our modeling techniques. In summary, this conference focused on the tools (detection, imaging techniques, modeling codes, computational power) as they are applied to interacting binaries, brown dwarfs, and exoplanets.

The main scientific highlight of the conference was that this goal was fully achieved. Consequently, most participants of the conference characterized it as extremely valuable and highly educational. There were 46 main lectures in addition to the opening lecture and two summary lectures, plus 57 three-minute mini-talks and 121 posters. Thirty-one countries were represented at the meeting. Also, 26% of the main speakers and 40% of the session chairs were female.

The conference was organized into eight scientific topics, complemented by an opening and a closing session. The scientific highlights of the individual sessions were:

Opening Lecture This lecture reviewed the modeling tools as well as several open problems in the field. As a result, an IAU Resolution will be drafted to adopt updated astrophysical parameters and constants to improve the accuracy of fundamental parameters. These include the use of GM(Sun) since this product is more accurate than the product of the separate quantities.

Multiwavelength Photometry and Spectroscopy of Interacting Binaries Several excellent review talks were presented about existing and future ground-based and space-based observational instruments devoted to a study of close binaries, with an overview of observational techniques and results. As a connection to exoplanet studies, one talk was devoted to the impact of CoRoT and Kepler on the close binary research. To provide a perspective for a future research, an extremely interesting talk was presented on planned Gaia and LSST missions.

Observations and Analysis of Exoplanets and Brown Dwarfs The session was opened by Didier Queloz, a co-discoverer of the first exoplanet orbiting a solar-type star. He summarized the present status of exoplanet search with an emphasis on the radial velocity techniques, and outlined the expected development of the field in the near future. The remaining talks concentrated both on exoplanets and brown dwarfs, emphasizing mostly the transiting planets observed by CoRoT and Kepler. There was also a very interesting talk which specifically described brown dwarfs in binary systems. Imaging Techniques for Binary Stars, Brown Dwarfs, and Exoplanets The highlights included several excellent reviews covering different topics of imaging: interferometry, Doppler tomography, polarimetry, vortex coronagraphy, nulling interferometry, adaptive optics, and direct imaging. A collection of talks on essentially all possible detection techniques was highly appreciated by the audience because it enabled the researchers to evaluate advantages and drawbacks of the individual techniques.

Model Atmospheres of Stars, Interacting Binaries, Disks, Exoplanets, and Brown Dwarfs This session was a collection of review talks devoted to modeling tools for the individual components of the close binary or exoplanetary systems - individual stars, planets, and accompanied disk-like structures. The talks summarized most of the currently used model atmospheres codes for computing LTE as well as non-LTE model atmospheres, model atmospheres of exoplanets, extended atmospheres with stellar winds, and 3-dimensional hydrodynamic simulations of stellar atmospheres. Several interesting new results were presented, for instance a possible use of accurately determined limb darkening coefficients for constraining basic stellar parameters.

Synthetic Light Curves, Velocity Curves, Spectra of Binary Stars, and Spectra of Binaries with Accretion Structures The new variants of the classical methods and programs for solving the light curves were discussed in this session, as well as the codes that aim at computing the spectrum of a complex close binary system by modeling in detail both stars and the circumstellar accretion structures around them. One of the main highlights was a presentation and statistical survey of a large number of the close binaries discovered by the Kepler mission.

Techniques for Analysis of Spectra and Light Curves The highlights of this session were two talks about two independent methods of spectral disentangling of the components of the binary system and their possible extensions to exoplanetary spectra. Other highlights included a talk on the history of the Rossiter-McLaughlin Effect followed by applications of the technique to transiting planets and low mass eclipsing binaries. In fact, this method represents the closest methodological connection between close binary and exoplanetary research. The effect was used earlier to identify critical properties of close binary systems, and it is now providing an analogously rich source of information in the case of exoplanets.

Formation and Evolution of Binary Stars, Brown Dwarfs, and Planets This session presented several excellent reviews on stellar evolution of the components of a close binary system, as well as dynamical models of formation and evolution of exoplanets. The highlights were a discussion and summary of non-conservative effects in the evolution of binaries, and a talk synthesizing simultaneous modeling of atmospheres and the global evolution of exoplanets.

Hydrodynamic Simulations of Exoplanets and Mass Transfer in Interacting Binaries The session dealt with close binary and exoplanet dynamics, including 3-dimensional hydrodynamic simulations of the atmospheres of these objects, and the mass transfer between them. The highlights were several simulations that showed the ever-increasing power of current numerical simulations to provide a detailed picture of mass transfer in the case of young binaries with low mass companions, common envelope binaries, and how magnetic fields influence cataclysmic variables and polars. One simulation also considered the meteorology of exoplanet atmospheres via models of global atmospheric circulations and transport of energy from the day to the night side for close-in giant exoplanets.

Summary Lectures There were two summarizing talks, one on observational techniques, and the other on the theoretical techniques. The latter talk, besides summarizing recent progress, concentrated on a detailed discussion of open problems in the theory and challenges for the future.

Panel Discussions Panel Discussions were held at the end of each day to summarize the lectures and to make proposals for enhancements to current techniques. Twelve influential astronomers who have contributed to the development of important modeling tools or who have provided insightful reviews of these developments were invited to participate in the symposium as distinguished panelists: France Allard, Alan Batten, Edwin Budding, Edward Devinney, Peter Eggleton, Artie Hatzes, Ivan Hubeny, Wilhelm Kley, Helmut Lammer, Albert Linnell, Virginia Trimble, and Robert E. Wilson. On the first day, they discussed the historical boundaries between stars, stellar remnants, brown dwarfs, and planets based on their masses, energy production processes, and evolutionary stages. It was an opportunity to re-examine these objects beyond the established ideology. On subsequent days, there were lively discussions of various topics presented during the day, with the enthusiastic participation of the audience.

Education and Public Outreach Event in Poprad The conference was advertised to the public on the TV radio, and in the newspapers. The public was specifically invited to attend a popular talk by Ivan Hubeny on “Detecting and Studying Extrasolar Planets,” in the Czech language (which is very close to the native Slovak language). The presentation was given in the Town Hall in the nearby city of Poprad, and it was well received by the public. Thirty-seven people attended the lecture and many of them asked questions.

Commemoration of the 110th Anniversary of the Birth of Dr. Antonín Bečvář An exhibition of several posters was prepared by Dr. Ladislav Hric to commemorate the 110th anniversary of the birth of Dr. Antonín Bečvář, founder of the Skalnate Pleso Observatory and author of several famous atlases and catalogues: Atlas Coeli, Atlas Borealis, Atlas Eclipticalis and Atlas Australis which were used nightly by astronomers around the world for almost half a century. The posters were displayed in the main conference lecture hall during the conference.

1. Meeting Number: 284

2. Meeting Title: The spectral energy distribution of galaxies

3. Coordinating Division: Division VIII (Galaxies and the Universe)

4. Dedication of meeting (if any): None

5. Location (city, country): Preston, UK

6. Dates of meeting: 5-9 September 2011

7. Number of participants: 151

8. List of represented countries: Argentina, Armenia, Australia, Belgium, Brazil, Canada, Cyprus, China, Croatia, Denmark, ESO, Finland, France, Germany, Greece, Italy, Japan, Mexico, New Zealand, The Netherlands, Portugal, Russia, , South Korea, Spain, Sweden, Switzerland, Taiwan, Thailand, UK, Ukraine, USA, Venezuela

9. Report submitted by: Cristina C. Popescu and Richard J. Tuffs

10. Date and place: Preston, UK Appendix 1: Scientific Program of IAU Symp. 284 Appendix 2: List of recipients of IAU grants Appendix 3: Scientific highlights of the meeting

A form for “Women in Astronomy” statistics was submitted to the Chair of “Women in Astronomy EC Working Group”.

11. Signature of SOC Chairperson: SED2011: The Spectral Energy Distribution of Galaxies (IAU Symposium 284, 5-9 September 2011, Preston, UK)

Programme Monday, Sept. 5th

Welcome and Introduction 09.00 - 09.10 Gordon Bromage Welcome Address (Chair: Richard Tuffs) 09.10 - 09.40 Barry F. Madore Introduction: The Reification of Galaxies: Cognitive Astrophysics and the Multiwavelength Inverse Problem

Session 1: Population Synthesis 09.40 - 10.20 IR Claus Leitherer Population Synthesis 10.20 - 10.40 CT Anne Sansom Effects of Non-Solar Abundance Ratios on Star Spectra: Comparison of Observations and Models 10.40 - 11.00 CT Philippe Prugniel High Spectral Resolution Models of Stellar Populations Resolved in Detailed Abundances 11.00 - 11.30 Coffee Break in the Poster Area 11.30 - 11.50 CT Daniel Schaerer The Importance of Nebular Emission for SED Modelling of Distant Star-forming Galaxies 11.50 - 12.10 CT Ignacio Ferreras Beyond Model Fitting SEDs 12.10 - 12.30 CT Sara Heap What the UV SED tells us about Unresolved Stellar Populations and Galaxies 12.30 - 12.50 CT Benjamin D. Johnson Star Formation History and the SED of Dwarf Galaxies: Insights from Resolved Stars

Lunch 12.50 - 14:10 Lunch and Poster Viewing (Coffee Available from 13:40 in the Poster Area)

Session 2: Understanding the Emergent SEDs Of Local Universe Galaxies (Chair: Kenny Wood) 14.10 - 14.40 IT Xander Tielens Chemical and Physical Properties of Interstellar Grains 14.40 - 15.20 IR Ralf Siebenmorgen Dust Processing of Radiation in Galaxies

Spiral And Dwarf Galaxies 15.20 - 15.40 CT Ilse De Looze A Detailed Energy Balance Study of the Sombrero Galaxy 15.40 - 16.00 CT Brent Groves Linking the Stars and Dust in M31 16.00 - 16.30 Coffee Break in the Poster Area 16.30 - 16.50 CT George Bendo Investigations of Dust Heating in M81, M83 and NGC 2403 with Herschel and Spitzer 16.50 - 17.10 CT Erin Mentuch How Stars Heat and Create the Dust in a Nearby Elliptical and Spiral Galaxy 17.10 - 17.30 CT Oskar Karczewski Modelling Blue Compact Dwarf Galaxies with MOCASSIN 17.30 - 17.50 CT Ciska Kemper Deconstructing the Spectral Energy Distribution of the Large Magellanic Cloud: Contributions from the Point Sources

19.00 - 20.30 Welcoming Reception at The Harris Museum Tuesday, Sept. 6th

Session 2: Understanding the Emergent SEDs of Local Universe Galaxies (continued)

Spiral and dwarf galaxies (continued) (Chair: Daniel Schaerer) 9.00 - 9.30 IT Suzanne Madden The Elusive ISM of Dwarf Galaxies: Assessing the Dust and Gas Properties in Low Metallicity Environments 9.30 - 9.50 CT Ute Lisenfeld The Dust SED in Dwarf Galaxies: The Case of NGC 4214 9.50 - 10.20 IT Sukanya Chakrabarti Spikes in the SED and Ripples in the Outskirts of Galaxies

Starburst Galaxies and AGN 10.20- 10.40 CT Gregory Snyder Modelling Bulge Assembly Through Galaxy Interactions 10.40 - 11.00 CT Lauranne Lanz The SEDs of Interacting Galaxies 11.00 - 11.30 Coffee Break (Chair: Barry Madore) 11.30 - 11.50 CT Andreas Efstathiou A New Model for the Infrared Emission of IRAS F10214+4724 11.50 - 12.10 CT Renee Kraan-Korteweg The SED of the Nearby HI-massive LIRG HIZOA J0836-43: from the NIR to the Radio Domain 12.10 - 12.50 IR Daniel Wang Emission Sources of X-rays from Galaxies 12.50 - 13.10 CT Almudena Prieto Optical-NIR/MIR Spectral Energy Distribution at Parsec Scales of the Nearest AGN

Lunch 13.10 - 14.30 Lunch and Poster Viewing (Coffee Available from 14:00 in the Poster Area)

(Chair: Ignacio Ferreras) 14.30 - 14.50 CT Mark Lacy SEDs of Dust-obscured selected in the Mid-infrared

Early-type Galaxies 14.50 - 15.20 - IT Martin Bureau Molecular Gas, Dust, and Star Formation in Early-type Galaxies 15.20 - 15.40 CT Hyunjin Jeong Young Stars in Nearby Early-type Galaxies: SED Fitting based on Ultraviolet (UV) and Optical Imaging 15.40 - 16.00 CT Richard McDermid Star Formation Histories of Early-Type Galaxies 16.00 - 16.30 Coffee Break in the Poster Area

(Chair: Patricia Sanchez-Blazquez) 16.30 - 16.50 CT Hidehiro Kaneda Dust and PAHs in X-ray of Elliptical Galaxies

Multiwavelength Surveys 16.50 - 17.10 CT Dave L. Clements Far-IR to Submm SEDs for Local Galaxies: Herschel, Planck and the HRS 17.10 - 17.30 CT Elisabete Da Cunha A Simple Model to estimate the Dust Content and Star Formation Activity of Galaxies from their observed SEDs 17.30 - 17.50 CT Denis Burgarella CIGALE: An UV-to-submm SED Fitting Code, Applications from the Local Universe to the Highest Redshift 17.50 - 18.10 CT Veronique Buat Fitting the full SED (from UV to Far-IR) of Galaxies: New Constraints on Dust Attenuation and Star Formation Determinations, from Z=0 to Z=2 Wednesday, Sept. 7th

Session 2: Understanding the Emergent SEDs of Local Universe Galaxies (continued)

Multiwavelength Surveys (continued) (Chair: Renee Kraan-Korteweg) 9.00 - 9.40 IR Simon Driver Panchromatic Properties of Galaxies in Wide-field Optical Spectroscopic and Photometric Surveys 9.40 - 10.00 CT Meiert Grootes Investigating Environmental Dependencies of Gas-Fuelling in GAMA Galaxies 10.00 - 10.20 CT John Moustakas PRIMUS - The PRIsm MUlti-object Survey 10.20 - 10.40 CT Viviana Acquaviva From Fluxes to Physical Properties: SED Fitting with Markov Chain Monte Carlo 10.40 - 11.00 CT Sharon Meidt The S4G View of Stellar Mass, MIR Dust, and Evolved, Intermediate-age Stars in Nearby Galaxies 11.00 - 11.30 Coffee Break in Poster Area 11.30 - 11.50 CT Steven Bamford Measuring SEDs for Individual Galaxy Components 11.50 - 12.10 CT Kyuseok Oh Improved and Quality-Assessed Emission and Absorption Line Measurements in Sloan Digital Sky Survey Galaxies

Session 3: Star-Formation in Galaxies 12.10 - 12.50 IR Bruce Elmegreen What Triggers Star-formation in Galaxies? 12.50 - 13.10 CT Hong-Xin Zhang Variations of the Star Formation Histories and the Stellar Mass of the LITTLE THINGS Dwarf Irregular Galaxies

Lunch 13.10 - 14.30 Lunch and Poster Viewing (Coffee Available from 14:00 in the Poster Area)

Session 3: Star-Formation in Galaxies (Chair: Hidehiro Kaneda) 14.30 - 14.50 CT Barry F. Madore Decoding the Schmidt Law 14.50 - 15.10 CT Yu Gao The Global Star Formation Law of Galaxies in Terms of Dense Molecular Gas 15.10 - 15.40 IT Francois Boulanger The Energetics of Turbulent Molecular Gas 15.40 - 16.00 CT Giovanni Natale The Nature of the Dust Emission in Stephan's Quintet 16.00 - 16.30 Coffee Break in Poster Area

(Chair: Daniel Wang) 16.30 - 17.00 IT Chris Martin "GALEX (Galaxy Evolution Explorer): Tracing Star Formation History using Spectral Energy Distributions 17.00 - 17.30 IT Andrew Hopkins Multiwavelength Indicators of SFR 17.30 - 18.00 IT Andreas Zezas Accreting Binaries and Star Formation in Galaxies 18.00 - 18.20 CT Stefano Zibetti Resolved Optical-infrared SEDs of Galaxies: Universal Relations and their Break-down on Local Scales Thursday, Sept. 8th

Session 4: The Panchromatic View Of The Milky Way (Chair: Francois Boulanger) 9.00 - 9.20 CT Jiali Zhu The Dust Temperature and ISRF in Hi-GAL SDP Fields 9.20 - 9.40 CT Kenny Wood 3D Radiation Transfer Modeling of Observations of Dust and Ionized Gas in the Galaxy 9.40 - 10.00 CT Norikazu Mizuno The CO View of the Milky Way by NANTEN 10.00 - 10.30 IT Brenda Dingus High Energy Imaging of the Milky Way 10.30 - 10.50 CT T. Porter Multi-Wavelength View of Cosmic-Ray Induced Diffuse Emissions from the Milky Way and Local Group Galaxies 10.50 - 11.20 Coffee Break in the Poster Area (Chair: Andreas Zezas) 11.20 - 11.40 CT Christoph Deil The HESS View of the Milky Way in TeV Light 11.40 - 12.10 IT Roland Crocker The Galactic Center - A Laboratory for Starburst Galaxies

Session 5: Linking Low and High-Energy Properties Of Galaxies

12.10 - 12.30 CT Kazufumi Torii Dark Gas: A new possible link between Low- and High-Energy Phenomena 12.30 - 13.00 IT Jim Hinton High-Energy Emission Mechanisms in Galaxies: Status, Prospects and Multi-wavelength Connections

Lunch 13.00 - 14.30 Lunch and Poster Viewing (Coffee Available from 14:00 in the Poster Area)

Session 5: Linking Low and High-Energy properties of Galaxies (continued) (Chair: Steven Serjeant) 14.30 - 14.50 CT Brian Lacki Cosmic Rays and High Energy Emission from Starburst Galaxies 14.50 - 15.10 CT W. Domainko Gamma Rays from the Starburst Galaxy NGC 253 15.10 - 15.40 IT Todd Thompson The Infrared Radio Correlation 15.40 - 16.00 CT F.S. Tabatabaei Resolved Radio-FIR/Submm Correlation in Nearby Galaxies with Herschel 16.00 - 16.30 Coffee Break in the Poster Area 16.30 - 16.50 CT Gustavo Romero The Non-thermal Broadband Spectral Energy Distribution of Radio Galaxies 16.50 - 17.10 CT Alberto Dominguez An Empirical Approach to the Extragalactic Background Light from AEGIS Galaxy SED-type Fractions

19:15 Guided Tour at The Hoghton Tower and Conference Dinner Friday, Sept. 9th

Session 5: Linking Low and High-Energy Properties Of Galaxies (continued) (Chair: David Clements) 9.00 - 9.30 IT Kalevi Mattila Photometric Measures of the Extragalactic Background Light 9.30 - 9.50 CT Yoshiki Matsuoka Cosmic Optical Background: The View from Pioneer 10/11 9.50 - 10.20 IT Luigi Costamante Constraints on IR Extragalactic Background Radiation from Veritas and HESS VHE Gamma-ray Absorption Studies

Session 6: Understanding The Cosmological Evolution Of Emergent SEDs 10.20 - 11.00 IR Michael Rowan-Robinson Panchromatic Radiation from Galaxies as a Probe of Galaxy Formation and Evolution 11.00 - 11.30 Coffee Break 11.30 - 11.50 CT T. Takagi Photometric Study of PAH Emission from Distant Infrared Galaxies 11.50 - 12.20 IT Loretta Dunne Digging Up the Dirt on Galaxies with Herschel 12.20 - 12.40 CT Stijn Wuyts Accurate SFRs and the Mode of Star Formation Over 11 Gyr of Lookback Time 12.40 - 13.00 CT Sugata Kaviraj The Star Formation Histories of Early-type Galaxies: New Insights from the Rest-frame Ultraviolet

Lunch 13.00 - 14.10 Lunch (Chair: Brad Gibson) 14.10 - 14.40 IT Martin Meyer Linking Gas Content and Star-formation Activity over Cosmic Time 14.40 - 15.00 CT Ray Norris EMU: The Evolutionary Map of the Universe 15.00 - 15.30 IT Steve Serjeant Multiwavelength Properties of Distant Lensed Galaxies 15.30 - 16.00 IT Asantha Cooray Multiwavelength Probes of the Epoch of Reionization 16.00 - 16.30 Coffee Break (Chair: Gordon Bromage) 16.30 Conference Summary Jay Gallagher, Gustavo Bruzual and Carol Lonsdale

Public Talk 19:00 Don Kurtz The Beauty of Galaxies: from the Milky Way to the Beginning of Time Poster contributions

Nicola Agius “Using GAMA and H-ATLAS data to explore the cold dust properties of Early-Type Galaxies”

Ellen Andrae “Probing the opacity of local Universe GAMA galaxies using attenuation-inclination relations from the UV to the near- IR”

Ko Arimatsu “Properties of Mid- to Far- Infrared Dust Emission in the Nearby Superwind Galaxy M82”

George J. Bendo “Extragalactic Science with ALMA”

Frederic Boone “The unusual multi-wavelength SED of optical-dropout galaxies”

Igor Chilingarian “NBursts+phot: parametric recovery of galaxy star formation histories from the simultaneous fitting of spectra and broad-band spectral energy distributions”

Laure Ciesla “The spectral energy distributions of the complete sample of the Herschel Reference Survey”

André de Castro Milone “An empirical spectrum library of chemically well characterized stars for stellar population modelling”

Guillaume Drouart “Decomposition of AGN and Stellar components in High redshift Radiogalaxies from redshift 1 to 5”

A. Eungwanichayapant “Synchrotron Radiation from Giant Electron/Positron Pair Halos”

Mercedes E. Filho “Optically Faint AGN in Galaxy Cluster Fields”

Nahiely Flores-Fajardo “Ionization of the diffuse gas in galaxies : Hot low-mass evolved stars at work” Anna Gallazzi “Charting the evolution of the ages and metallicities of the massive galaxy population since z=0.7 with optical spectroscopy”

Frederic Galliano “Non-Standard Grain Properties, Massive Dark Gas Reservoir, and Extended Submm Excess, Probed by Herschel in the LMC”

Jean Michel Gomes “Stellar populations in the centers of nearby galaxies”

Jean Michel Gomes “Spectral Fitting of SDSS Passive Galaxies with alpha-enhanced Single Stellar Population”

Lucia Guaita “Spectral energy distribution properties of z~2 star forming galaxies”

Philip Günster “Spectroscopic features of the superthin LSB galaxy UGC12281”

C. Henkel “A CO J=3-2 Survey of Galaxies - Implications for Molecular SEDs”

Israel Hermelo “Modelling the dust heating and emission in the dwarf galaxy NGC 4214”

Benne W. Holwerda “NHMESES and HEROES observations of NGC 4244 and NGC 891”

Benne W. Holwerda “Looking at the distant Universe with the MeerKAT Array (LADUMA)”

Noelia Jiménez “The impact of thermally pulsing asymptotic giant branch stars on the red sequence of clusters galaxies”

Hidehiro Kaneda “The next-generation infrared astrnomoy mission SPICA”

Ivan Katkov “Multi-component parametric inversion of galaxy kinematics and stellar populations using full spectral fitting” Mina Koleva “Stellar population models in the blue”

Ralf Kotulla “Using GALEV and photometric redshifts to study galaxy evolution”

Man I Lam “The Preliminary results on morphological IR relation on GAMA Galaxies in the Hershel ATLAS Field”

Yoshiki Matsuoka “Cosmic Optical Background: the View from Pioneer 10/11”

S. Meneses-Goytia “Spectral Energy Distributions of Single Stellar Populations in the Infrared range”

Leão Souza João Rodrigo “A Spitzer Study of Interacting Luminous and Ultra-Luminous Infrared Galaxies”

Jaehyun Lee “Does the SED of a galaxy constrain its merger history?”

Lijie Liu “The Global Star Formation Law of Galaxies Revisited in the Radio Continuum”

Carol Lonsdale “Feedback from the most luminous dust-obscured AGNs in the universe”

Nidia Lugo “Model for simulate the Temporal Evolution of the Hα Luminosity, FUV and NUV flux of Stellar Population of a Galaxy”

W. J. Maciel “The star formation rate in the Milky Way: results from stars and planetary nebulae”

John MacLachlan “The Dust Distribution in Late Type Low Surface Brightness Disks”

Gladis Magris C. “A new bayesian approach to quantify the uncertainties in the determination of galaxy properties derived from spectral fits” Minnie Mao Yuan “No Evidence for Evolution in the Far-Infrared Radio Correlation out to z~2 in the eCDFS”

A. M. Mickaelian “Spectral Energy Distribution and classification of bright active galaxies”

Danielle M. Nielsen “The current star formation rate of K+A galaxies”

R. A. Ortega-Minakata “What makes a galaxy radio loud?”

Bogdan Adrian Pastrav “Dust effects on the derived photometric parameters of disks and bulges in spiral galaxies”

Ando Lalaina Ratsimbazafy “Age-dating Stellar populations of Luminous Red Galaxies”

Mónica Relaño “SED analysis of HII regions in M33”

Aurélie Rémy “Characterising the FIR/submm Emission of Dwarf Galaxies : First Results of the Herschel Key Program, The Dwarf Galaxies Survey”

Myriam Rodrigues “Retrieve stellar populations in starbursts”

Kate Rowlands “H-ATLAS/GAMA: A multiwavelength view of dusty early-type galaxies and passive spirals”

Paul Ruffle “Identification of mid-infrared point sources in the Magellanic Clouds”

David Sanchez “The challenging SED of AP Librae (PKS1514-241)”

Patricia Sanchez-Blazquez “The SFH of disk galaxies”

Andrew Schechtman-Rook “The 3-Dimensional Structure of NGC 891” Chris Sedgwick “Optical Spectroscopy of Far-infrared Sources in the AKARI/Spitzer/Herschel near-SEP Deep Field”

Kwang-il Seon “Detection of a Large Amount of Diffuse Extraplanar Dust in NGC 891”

Zhengyi Shao “Constrain the stellar population gradients of elliptical galaxies with SED”

Olga K. Silchenko “Outer disks of lenticular galaxies”

Dan Smith “The SEDs of galaxies selected at 250um”

Laura K. Sturch “TYPHOON Observations of the Lindsay-Shapley Ring”

Toyoaki Suzuki “AKARI observations of the multiphase intergalactic medium of Stephan's Quintet”

Ryan Swindle “Measuring Systematic Effects in Early-Type Galaxy Stellar Masses from Photometric SED Fitting”

F.S. Tabatabaei “Variation in the dust emissivity index across M33 (HerM33es)”

Qinghua Tan “High Resolution SMA Imaging of (Ultra)-Luminous Infrared Galaxies”

Tomislav Terzic “Multiwavelength observations of the radio 4C 21.35”

Yoshiki TOBA “The Mid-Infrared Luminosity Function of Galaxies by using AKARI mid-infrared All-Sky Survey Catalogue”

Tova Yoast-Hull “Cosmic Ray Production and Emission in M82”

Jing Wang “Inside-out disk formation and subsequent bar-driven evolution in the local universe” Sukyoung Yi “UV upturn as a test for Helium Sedimentation in Dark Halo Evolution”

Fang-Ting Yuan “Mid-infrared and Star Formation Properties from the Spectral Energy Distribution (SED) of Galaxies”

O. V. Zakhozhay “The Results of SEDs Modeling for Substars with Protoplanetary Disks”

Zhiyu Zhang “Multiple CS line survey in local star-forming galaxies”

Stefano Zibetti “Direct constraints on the impact of TP-AGB stars on the SED of galaxies from NIR spectroscopy”

SED2011 List of Participants Surname Forename Country Gender Acquaviva Viviana USA Female Agius Nicola UK Female Andrae Ellen Germany Female Arimatsu Ko Japan Male Bamford Steven UK Male Bendo George UK Male Boulanger Francois France Male Bromage Gordon UK Male Bruzual Gustavo Venezuela Male Buat Veronique France Female Bureau Martin UK Male Burgarella Denis France Male Chakrabarti Sukanya USA Female Chilingarian Igor Russia Male Clarke Adam UK Male Clements David UK Male Clowes Roger UK Male Cooray Asantha USA Male Costamante Luigi Italy Male Crocker Roland Germany Male da Cunha Elisabete Germany Female De Castro Milone Andre Brazil Male De Looze Ilse Belgium Female Deil Christoph Germany Male Dingus Brenda USA Female Dominguez Alberto USA Male Driver Simon Australia Male Drouart Guillaume ESO Male Dunne Loretta New Zealand Female Efstathiou Andreas Cyprus Male Elkin Vladimir UK Male Elmegreen Bruce USA Male Eungwanichayapant Anant Thailand Male Ferreras Ignacio UK Male Filho Mercedes Portugal Female Flores-Fajardo Nahiely Mexico Female Gallagher John (Jay) USA Male Gallazzi Anna Denmark Female Galliano Frederic France Male Gao Yu China Male Gibson Brad UK Male Gomes Jean Michel Portugal Male Grootes Meiert Willem Germany Male Groves Brent Germany Male Guaita Lucia Sweden Female Günster Philip Germany Male Hambleton Kelly UK Female Harvey Paul USA Male Hassall Barbara UK Female SED2011 List of Participants

Heap Sara USA Female Henkel Christian Germany Male Hermelo Israel Spain Male Hinton Jim UK Male Holwerda Benne Netherlands Male Hopkins Andrew Australia Male Jeong Hyunjin South Korea Male Jiménez Noelia Argentina Female Johnson Benjamin France Male Jones David Germany Male Kaneda Hidehiro Nagoya Male Karczewski Oskar UK Male Katkov Ivan Russia Male Kaviraj Sugata UK Male Kemper Ciska Taiwan Female Koleva Mina Belgium Female Kotulla Ralf USA Male Kraan-Korteweg Renée C. South Africa Female Kurtz Don UK Male Lacki Brian USA Male Lacy Mark USA Male Lam Man I China Female Lanz Lauranne USA Female Lee Jaehyun South Korea Male Leitherer Claus USA Male Lisenfeld Ute Spain Female Liu Lijie China Female Lonsdale Carol USA Female Lugo Nidia Venezuela Female Maciel Walter Brazil Male MacLachlan John UK Male Madden Suzanne France Female Madore Barry USA Male Magris Crestini Gladis Venezuela Female Mao Minni Australia Female Martin Christopher USA Male Matsuoka Yoshiki Japan Male Mattila Kalevi Finland Male Maxwell Michael UK Male McDermid Richard USA Male Meidt Sharon Germany Female Meneses-Goytia Sofia The Netherlands Female Mentuch Erin Canada Female Meyer Martin Australia Male Mickaelian Areg Armenia Male Mizuno Norikazu Japan Male Moustakas John USA Male Murphy Simon UK Male Natale Giovanni UK Male Nielsen Danielle USA Female SED2011 List of Participants Norris Ray Australia Male Oh Kyuseok South Korea Male Ortega-Minakata Rene A. Mexico Male Pastrav Bogdan Adrian UK Male Pilkington Kate UK Female Popescu Cristina UK Female Porter Troy USA Male Prieto Almudena Spain Female Prugniel Philippe France Male Ratsimbazafy Ando South Africa Female Relano Pastor Monica Spain Female Remy Aurelie France Female Romero Gustavo E. Argentina Male Rowan-Robinson Michael UK Male Rowlands Kate UK Female Ruffle Paul UK Male Sanchez David Germany Male Sanchez-Blazquez Patricia Spain Female Sansom Anne E. UK Female Schaerer Daniel Switzerland Male Schechtman-Rook Andrew USA Male Sedgwick Chris UK Male Seon Kwang-il South Korea Male Serjeant Stephen UK Male Shao Zhengyi China Male Siebenmorgen Ralf ESO Male Silchenko Olga Russia Female Smith Daniel UK Male Snyder Gregory USA Male Souza Leão João Rodrigo Brazil Male Sturch Laura USA Female Suzuki Toyoaki Japan Male Swindle Ryan USA Male Tabatabaei Fatemeh Germany Female Takagi Toshinobu Japan Male Tan Qinghua China Female Terzić Tomislav Croatia Male Thompson Todd USA Male Toba Yoshiki Japan Male Torii Kazufumi Japan Male Tuffs Richard Germany Male Wang Jing Germany Female Wood Kenny UK Male Wuyts Stijn Germany Male Yoast-Hull Tova USA Female Yuan Fang-Ting Japan Female Zakhozhay Olga Ukraine Female Zezas Andreas Greece Male Zhang Hong-Xin USA Male Zhang Zhiyu Germany Male SED2011 List of Participants Zhu Jiali China Female Zibetti Stefano Denmark Male Scientific Highlights of IAU Symposium 284

IAU Symposium 284, jointly organised by the University of Central Lan- cashire (Preston) and the Max-Plank Institut f¨ur Kernphysik (Heidelberg), brought together developers and users of self-consistent physical or semi- empirical models for the emergent panchromatic spectral energy distribu- tions (SEDs) of galaxies ranging over the complete accessible spectral range from gamma-rays to radio. Motivated by the rapid developmentinthecor- responding observational capabilities in the last decade, the main goal of the symposium was to provide a forum for the interaction of modellers with both observers assembling multiwavelength datasets on galaxiesandtheoreticians considering fundamental physical processes in galaxies. The program was fashioned to reflect the interconnections between the very broad range of physical processes responsible for the panchromatic pho- ton output of galaxies. This embraced the formation, evolution and emission of stars; accretion-driven sources of photons; the chemicalandphysicalprop- erties of the interstellar medium, including both the gaseous and solid-state components and their interactions with ambient photon fields; and high en- ergy processes involving cosmic rays. On the last day a final session was dedicated to models for the evolution of the panchromatic SEDs of galaxies over cosmological time, thus linking the detailed physical processes in indi- vidual galaxies discussed earlier in the week with the photonoutputofthe Universe. All of these topics have, of course, been the subjects of many dedicated individual symposia in the past, attended largely by their own specialized communities. However, IAU symposium 284 was unique in its concept of connecting the topics and bringing together the communities(oratleastmak- ing a significant step towards achieving this). A particular challenge of this concept was to avoid the symposium becoming a sequence of self-contained mini-workshops on each of the constituent topics, addressing selected topical issues directed at, and attended by, one particular community. However, in this respect any prior concerns proved to be completely unfounded. All the delegates, representing a mix of theoreticians, observers,andspecialistsin the many technical and astrophysical subfields needed to build SED models, proved to be enthustiastic and proactive participants throughout the week, generating many perceptive, and sometimes unexpected interdiscipinary dis- cussions following both the oral presentations (many of these discussions could be documented for inclusion in the proceedings) and in the poster

1 sessions. There were no parallel sessions. In general, the intellectual at- mosphere was open and constructive, with several known examples of new collaborations arising from discussions initiated at the symposium. For this, particular thanks must go to the authors for their careful preparation of the presentations. These were generally well directed to the broad audience, while very effectively answering the call for papers to highlight techniques and results combining measurements made from across the electromagnetic spectrum. Indeed, this response to the symposium confirms thegenuineneed and demand for more effective quantitative analysis techniques to exploit the already copious amounts of multwavelength data now available for galaxies near and far. The open and exploratory tone for the symposium was set by the intro- ductory review by Barry Madore (“The Reification of Galaxies:Cognitive Astrophysics and the Multiwavelength Inverse Problem”) which, using exam- ples from everyday life and the art world as well as from astrophysics, was a thought-provoking philosophical discourse on the extent towhichastrophysi- cists can ever hope to extract a “true and complete” understanding of galaxies based on the unavoidably biased viewpoints available to us. Throughout the succeeding sessions, many examples of this fundamental issue emerged, both positive, in the sense of a different (and perhaps better informed) picture emerging from a multiwavelength view, and negative, in the sense that we may not have been aware, or cannot easily observationally constrain, some fundamental property shaping galaxian SEDs. A vivid (and, tomany,unex- pected) example of the latter was contained in the review by Claus Leitherer on population synthesis, which emphasised that the effectivetemperature,lu- minosity and ionising radiation of massive stars was strongly dependent not only on mass and metallicity, but also on the rotation of the stars. Examples of the former came in several presentations showing impressive comparisons between the observed UV/optical-FIR/submm emission of various types of galaxies and AGN, and predictions based on radiation transfer calculations. Aparticularhighlightofthemeetingwasthesessionlinkinglow-and high-energy properties of galaxies. Although mainly confined to the Milky Way (included as a separate topic for this reason) and the two starburst galaxies already detected in gamma-rays by ground and space-borne facili- ties, the session confirmed the very rich potential of a combined analysis of the radio tracers of interstellar gas, infrared/optical tracers of photon fields and dust column, and the low and high energy gamma-ray tracers of gas and cos- mic ray electrons and protons. Various presentations showednewmodelling

2 results on different aspects of this, connecting issues such as the nature of the so-called “dark gas”, the emissivity of grains, the energy-dependent propaga- tion of cosmic rays (both within gas clouds and on galaxy-widescales),and the strength of ambient magnetic fields. The invited talk of Luigi Costamante in the same session also considered the impact of gamma-ray astronomy on inferences of the UV/optical/infrared emission of the ensemble of distant galaxies, as derived from the attenuation of TeV emission from blazars by pair production in the intergalactic radiation field. This could be compared and contrasted with inferences from direct observations of the extragalactic background light in the UV/optical/infrared, reviewed by Kalevi Mattila, as well as with constraints from theoretical modelling of blazar SEDs. This led on to a detailed consideration of the panchromatic radiationfromgalaxies as a probe of galaxy formation and evolution by Michael Rowan-Robinson, with strong physical insights to the field. The symposium was attended by participants from 33 different coun- tries from Europe, North America, South America, Asia, Africa and Aus- tralia/Oceania, with a balanced representation between , senior scientists and young career scientists, postdoctoral fellows and PhD students. This large variety of scientists from all continents, at different stages in their career and professional achievements, together with the interdisciplinary na- ture of the meeting led to a fantastic scientific interaction between delegates, as documented in the written feedback received from the participants. The large and international attendance of the Symposium, as well as the prestige brought by the invited speakers and members of the SOC attracted alotofpublicattentioninLancashire.Thiswasreflectedbythe impressive attendance of the public talk by Prof. Don Kurz from the University of Central Lancashire, on “The Beauty of Galaxies: from the Milky Way to the Beginning of Time”, organised on the occasion of IAU Symp. 284. The participants of the symposium very much appreciated the visit and guided tour to the beautiful “Houghton Tower”, with history dating back to the Norman Conquest, and whose famous guests had included William Shakespeare, Charles Dickens and King James I. The conference banquet was held in the main hall of the Tower, in the same room (and, formembers of the SOC at the very same same oak table) where King James I, ata banquet held in his honour, famously knighted a loin of beef “Sir Loin”, four hundred years previously.

3 International Astronomical Union U n i o n A s t r o n o m i q u e I n t e r n a t i o n a l e POST MEETING REPORT FORM for meetings other than Joint Discussions and Special Sessions Deadline for Submission: within 1 month after the meeting the following information should be sent to the IAU Assistant General Secretary

The following documents should be attached:

i. Final Scientific Program ii. List of participants iii. List of recipients of IAU Grants, including amount and country iv. Receipts signed by the recipients of IAU Grants (This does not apply to Scientific Meetings held during General Assemblies) v. Brief report (text.txt file or word.doc) to the Executive Committee on the scientific highlights of the meeting (1-2 pages)

1. Meeting Number: IAU Symposium 285 2. Meeting Title: New Horizons in Time Domain Astronomy 3. Coordinating Division: XII (Commission 5) 4. Dedication of meeting (if any): 5. Location (city, country): Oxford, UK 6. Dates of meeting: September 19-23, 2011 7. Number of participants: 239 (22% women, 78% men) 8. List of represented countries: 1. Armenia (1) 2. Australia (11) 3. Austria (1) 4. Belgium (4) 5. Brazil (1) 6. Bulgaria (2) 7. Canada (10) 8. Chile (2) 9. China (2) 10. Denmark (1) 11. Finland (1) 12. France (3) 13. Georgia (1) 14. Germany (7) 15. Hungary (2) 16. India (1) 17. Ireland (3) 18. Israel (4) 19. Italy (4) 20. Japan (5) 21. Korea (1) 22. Netherlands (9) 23. Poland (1) 24. Russia (2) 25. South Africa (7) 26. Spain (6) 27. Sweden (1) 28. Switzerland (5) 29. Ukraine (2) 30. UK (52) 31. USA (87) 9. Report submitted by: Elizabeth Griffin, Robert Hanisch, Co-Chairs of SOC 10. Date and place: March 23, 2012, Victoria, BC, Canada and Baltimore, MD, USA 11. Signature of SOC Chairperson:

Symposium

Schedule

New Horizons in Time Domain Astronomy, th rd Oxford September 18 -23 2011

SUNDAY, September 18th, 2011: Opening reception and conference registration 6:30 pm – 8.30 pm Opening reception and conference registration Denys Wilkinson Building, Keble Road

Invited talks (I) are 20 minutes + 5 minutes for questions Contributed talks (C) are 12 minutes + 3 minutes for questions

MONDAY, September 19th, 2011: “Can our data meet the challenges?” 8:00 am – 4:00 pm REGISTRATION

8:45am – 9:05 am Welcome to Oxford: The Lord Mayor of Oxford, Cllr. Elise Benjamin, and Prof. Roger Davies, Head of Oxford Astrophysics Prof. Bob Hanisch (Co-chair, SOC)

9:05 am – 9.35 am KEYNOTE ADDRESS: Brian Warner: “The power of the unexpected”

9:35 am – 10:25 am PLENARY SESSION ONE (Chair: Bob Hanisch)

09:35am Brian Schmidt (I): “New wide-field optical surveys” 10:00am Rob Fender (I): “The scientific potential of LOFAR”

10:25 am – 10:55 am COFFEE/TEA

10:55 am – 1.00 pm PLENARY SESSION TWO (Chair: Rob Seaman)

10:55am Hans Kjeldsen (I): “CoRoT, MOST, and Kepler” 11:20am Josh Grindlay (I): “Opening the 100yr time domain astronomy window with DASCH” 11:45am Phil Charles (I): “Long-term Monitoring with Small and Medium-sized Telescopes on the Ground and in Space” 12:10pm Francesca Primas (I): “Spectroscopic surveys” 12:35pm Neil Gehrels (I): “Swift and Fermi Time Domain Astronomyy”

1:00 pm – 2:00 pm LUNCH BREAK

2:00 pm – 3:30 pm Workshops and break-out sessions – see separate programme

3:30 pm – 4:00 pm COFFEE/TEA

4:00 pm – 5:00 pm Workshops and break-out sessions – see separate programme

5:30 pm – 6:30 pm RECEPTION HOSTED BY THE LORD MAYOR OF OXFORD, TOWN HALL

7:30 pm – 9:00 pm PUBLIC LECTURE Prof. Martin Rees: “From microseconds to aeons - How our complex cosmos emerged” Oxford University Museum of Natural History; tickets required TUESDAY, September 20th, 2011: “Explosive or irreversible changes” 8:30 am – 4:00 pm REGISTRATION

09:00 am – 10:35 am PLENARY SESSION THREE (Chair: Mark Sullivan)

09:00am Jim Cordes (I): “The dynamic radio sky” 09:25am Shri Kulkarni (I): “Explosive events in the cosmos” 09:50am Mansi Kasliwal (C): “Systematically bridging the gap between novae and supernovae” 10:05am Howard Bond (C): “Intermediate-luminosity red transients” 10:20am Isobel Hook (C): “Transients with Euclid and the E-ELT”

10:35 am – 11:05 am COFFEE/TEA

11:05 am – 12.45 pm PLENARY SESSION FOUR (Chair: Tara Murphy)

11:05am Lars Bildsten (I): “Explosions on a variety of scales” 11:30am Stephen Smartt (I): “Transients with Pan-STARRS-1” 11:55am Armin Rest (C): “Light echoes of transients and variables” 12:10pm Brad Cenko (C): “A new class of relativistic outbursts from the nuclei of distant galaxies” 12:25pm Joe Lazio (C): “EM counterparts to LIGO-VIRGO events: EVLA observations”

12:45 pm – 2:00 pm LUNCH BREAK

2:00 pm – 3:30 pm Workshops and break-out sessions – see separate programme

3:30 pm – 4:00 pm COFFEE/TEA

4:00 pm – 5:30 pm Workshops and break-out sessions – see separate programme

WEDNESDAY, September 21st, 2011: “Things that tick” 8:30 am – 12:00 pm REGISTRATION

9:00 am – 10:30 am PLENARY SESSION FIVE (Chair: Patricia Whitelock)

09:00am Ben Stappers (I): “Pulsars” 09:25am Jason Hessels (C): “Charting the radio sky on sub-second time scales with LOFAR” 09:40am Don Kurtz (I): “Asteroseismology” 10:05am Roger Griffin (I): “Radial velocities: new science and new trends”

10:30 am – 11:00 am COFFEE/TEA

11:00 am – 1.00 pm PLENARY SESSION SIX (Chair: Keith Horne)

11:00am (I): “Probing the physics of planets and stars with transit data” 11:25am A. S-Czerny (I): “Sensitivity of Period Search” 11:50am Tom Loredo (C): “Steps, sines, and droplets: Semiparametric Bayesian modeling of arrival time series” 12:05pm Rebekah Hounsell (C): “Variable stellar object detection and light curves from the solar mass ejection imager” 12:20pm Arne Henden (C): “Surveying the bright sky” 12:35pm Barry Welsh (C): “High time resolution astronomy on the SALT 10m”

1:00 pm CONFERENCE PHOTO

FREE AFTERNOON

THURSDAY, September 22nd, 2011: “Irregular and aperiodic changes” 8:30 am – 5:00 pm REGISTRATION

8:45 am – 10:20 am PLENARY SESSION SEVEN (Chair: Arne Henden)

08:45am Erin Bonning (I): “AGNs, blazars, QSOs” 09:10am Stefano Ciprini (C): “Gamma-ray waveband and multi-waveband variability of blazars” 09:25am Keith Horne (C): “Echo mapping of AGN” 09:40am Franz Kerschbaum (I): “Variable red giants” 10:05am Geoffrey Clayton (C): “Two centuries of observing R Coronae Borealis”

10:20 am – 10:50 am COFFEE/TEA

10:50 am – 1:00 pm PLENARY SESSION EIGHT (Chair: Aris Karastergiou)

10:50am Rachel Osten (I): “Probing magnetic mysteries with stellar flares” 11:15am Isabelle Baraffe (I): “Stellar evolution in 3D” 11:40am Stephen Potter (I): “Polarimetric variability” 12:05pm Mark Walker(I): “Microscopy of the Interstellar Medium” 12:30pm Hayley Bignall (C): “The extreme scintillating quasar PKS 1257-326 revisited: What have we learned?” 12.45pm W. L. Diaz Merced (C): “Sonification prototype for 2D data analysis”

1:00 pm – 2:15 pm LUNCH BREAK

2:15 pm – 3:45 pm Workshops and break-out sessions – see separate programme

3:45 pm – 4:15 pm COFFEE/TEA

4:15 pm – 5:45 pm Workshops and break-out sessions – see separate programme

7:15 pm (for 7.30pm) CONFERENCE DINNER, WADHAM COLLEGE

FRIDAY, September 23rd, 2011: “Preparing for the future” 8:30 am – 12:00 pm REGISTRATION

9:00 am – 10:30 am PLENARY SESSION NINE (Chair: Brian Schmidt)

09:00am George Djorgovski (I): “Science strategies of synoptic sky surveys” 09:25am Laurent Eyer (I): “From Hipparcos to GAIA” 09:50am Michael Kramer(I): “Pulsars, SKA and Time Domain Studies in the Future” 10:15am J-P. Macquart (C): “Optimal strategies for transient surveys with wide field radio telescopes”

10:30 am – 11:00 am COFFEE/TEA

11:00 am – 12.55 pm PLENARY SESSION TEN (Chair: Elizabeth Griffin)

11:00am Lucianne Walkowicz (I): “The Future of the Time Domain with LSST” 11:25am Nicholas White (I): “Next-generation X-ray astronomy” 11:50am 5min Workshop Summaries and “Breaking News”

1:00 pm – 2:15 pm LUNCH BREAK

2:15pm Josh Bloom (I): “Technical and observational challenges for exploration of the time domain in the future” 2:40pm Rosemary Wyse (I): “Conference summary” 3:05pm DISCUSSION

3:30 pm – 4:00 pm COFFEE/TEA

END OF SYMPOSIUM

Schedule(for(afternoon(workshops(and(breakout(sessions( (( Lecture(Theate( JCR( Room(A( Room(C( Room(D( (( !! !! !! !! !! Monday( The!CoRoT!and!Kepler! SWIFT:!Opportunities,! Optical/NIR!transient! 2pm( Revolution!in!Stellar! Capabilities,!and!Data! Gravitational!Waves!(I)! !! surveys!(I)! (90min)( Variability!Studies! Handling!

Monday( Optical/NIR!transient! Communicating!stellar! 4pm( !! Gravitational!Waves!(II)! !! surveys!(II)! variability! (60min)( (( !! !! !! !! !! Tuesday( Using!the!VO!to!Study!the! 2pm( Extreme!physics!(I)! XKRay!Transient!surveys! Gravitational!Microlensing! Light!Echoes! Time!Domain!(I)! (90min)(

Tuesday( Small!and!Robotic! Binarity!and!Stellar! Using!the!VO!to!Study!the! 4pm( Extreme!physics!(II)! Astrotomography! Telescopes! Evolution! Time!Domain!(II)! (90min)( (( !! !! !! !! !! Historical!Time!Domain! Thursday( Algorithms!for!Time!Series! Astronomy!Data,! 2.15pm( Faint!and!Fast!Transients! Tidal!Disruption!Flares!(I)! Radio!Transients!(I)! Analysis!(I)! Processing!and! (90min)( Distribution! Data!Management,! Thursday( Algorithms!for!Time!Series! Infrastructure,!and! The!Amateur!Community! 4.15pm( Tidal!Disruption!Flares!(II)! Radio!Transients!(II)! Analysis!(II)! Archiving!for!Time!Domain! and!Citizen!Science!! (90min)( Science! (( !! !! !! !! !! All(room(allocations( Room( Main!Theatre:!240! JCR!lecture!theatre:!100! ! ! Capacities( are(provisional( Room!A:!50! Room!C:!50! Room!D:!40! ! !

IAU 285 Participant Summary

Name Affiliation Country 1 Suzanne Aigrain UK 2 Anastasia Alexov University of Amsterdam / API Netherlands 3 Richard I. Anderson Geneva Observatory Switzerland 4 Iair Arcavi Weizmann Institute of Science Israel 5 Carles Badenes University of Pittsburgh USA 6 Raymundo Baptista Universidade Federal de Santa Catarina Brazil 7 Isabelle Baraffe UK 8 Cesare Barbieri University of Padova Italy 9 Tom Barclay NASA Ames Research Center USA 10 Paul Beck Univ. Leuven Belgium 11 Andy Becker University of Washington USA 12 Timothy C. Beers Michingan State University and JINA USA 13 Guillaume Belanger ESAC, European Space Agency Spain 14 University of Oxford UK 15 Vasily Belokurov IoA, Cambridge UK 16 József Benkő Konkoly Observatory Hungary 17 Misty Bentz Georgia State University USA 18 David Bersier Liverpool John Moores University UK 19 Steven Bickerton Princeton University USA 20 Hayley Bignall ICRAR ‐ Curtin University Australia 21 Lars Bildsten Kavli Institute for Theoretical Physics, UC Santa Barbara USA 22 Sarah Blake University of Oxford UK 23 Josh Bloom UC Berkeley USA 24 Katherine Blundell Oxford Astrophysics UK 25 Mike Bode Liverpool JMU UK 26 Howard E Bond Space Telescope Science Institute USA 27 Erin Bonning Yale University USA 28 Regis Cartier Universidad de Chile Chile 29 Brad Cenko University of California, Berkeley USA 30 Joan Centrella NASA's Goddard Space Flight Center USA 31 Seo‐Won Chang Department of Astronomy, Yonsei University, Korea Korea 32 Phil Charles SAAO/UCT/Southampton South Africa 33 Eric Chassande‐Mottin APC CNRS Univ Paris Diderot France 34 Doron Chelouche Haifa University Israel 35 Anton Chernenko Space Research Institute Russia 36 Stefano Ciprini ASI Science Data Center & INAF Roma Observatory Italy 37 Geoff Clayton Louisiana State University USA 38 Susan Collins NUI Galway Ireland 39 Chris Copperwheat University of Warwick UK 40 Stephane Corbel University Paris Diderot & CEA Saclay France 41 Jim Cordes Cornell University USA 42 Kevin Covey Cornell University USA 43 Steve Croft UC Berkeley USA 44 Nick Cross IfA, Edinburgh UK 45 Maria Cruz Science Magazine UK 46 Jan Cuypers Royal Observatory of Belgium Belgium 47 James Davenport University of Washington USA 48 Ed Daw The University of Sheffield UK 49 Deanne de Bude University of Cape Town South Africa 50 Diarmaid de Burca National University of Ireland,Galway Ireland 51 Pieter Degroote Instituut voor Sterrenkunde Belgium 52 Wanda L. Diaz Merced University of Glasgow UK 53 George Djorgovski Caltech USA 54 Andrew Drake Caltech USA 55 Pierre Dubath Geneva Observatory Switzerland 56 Alessandro Ederoclite Instituto de Astrofísica de Canarias Spain 57 Peter Eggleton LLNL USA 58 Tom Evans Oxford University UK 59 Laurent Eyer Geneva Observatory Switzerland 60 Stephen Fairhurst Cardiff University UK 61 Glennys Farrar University USA 62 Rob Fender University of Southampton UK 63 Matilde Fernandez Institute de Astrofisica de Analucia Spain 64 Helene Flohic Universidad de Chile Chile 65 Boris Gaensicke University of Warwick UK 66 Bryan Gaensler CAASTRO / U. Sydney Australia 67 Jonathan Gair University of Cambridge UK 68 Neil Gehrels NASA/GSFC USA 69 Luis J. Goicoechea University of Cantabria Spain 70 Matthew Graham California Institute of Technology USA 71 Elizabeth Griffin HIA/DAO Canada 72 Roger Griffin Cambridge UK 73 Sean C. Griffin McGill University Canada 74 Josh Grindlay Harvard University USA 75 Ellie Hadjiyska Yale University USA 76 Daryl Haggard Northwestern University/CIERA USA 77 Pasi Hakala FINCA, U.of Turku Finland 78 Paul Hancock SIfA, The University of Sydney Australia 79 Robert Hanisch STScI/VAO USA 80 Patrick Hartigan Rice University USA 81 Kazuhiro Hayama NAOJ Japan 82 Arne Henden AAVSO USA 83 Jason Hessels ASTRON Netherlands 84 Tom Hettinger Michigan State University USA 85 Ian Heywood University of Oxford UK 86 Eric Hilton Univ. of Hawaii USA 87 Wynn Ho University of Southampton UK 88 Simon Hodgkin IoA, Cambridge UK 89 Doug Hoffman IPAC/Caltech USA 90 Isobel Hook U. Oxford and INAF Obs. Rome Italy 91 Keith Horne SUPA St Andrews UK 92 Rebekah Hounsell Liverpool John Moores University UK 93 Ted Jaeger NRL USA 94 Dayton Jones JPL USA 95 Derek Jones Institute of Astronomy, Cambridge UK 96 Noé Kains ESO Germany 97 Aris Karastergiou Oxford University UK 98 Sergey Karpov SAO of Russian Academy of Sciences Russia 99 Mansi M. Kasliwal Carnegie Observatories & Princeton University USA 100 JJ Kavelaars Herzberg Institute of Astrophysics Canada 101 Evan Keane Max Planck Institute for Radio Astronomy Germany 102 Franz Kerschbaum Univ. Vienna Austria 103 Michael Kesden New York University USA 104 Dae‐Won Kim Harvard‐Smithsonian CfA USA 105 Oliver King Caltech USA 106 Hans Kjeldsen Aarhus University Denmark 107 Katrien Kolenberg Harvard‐Smithsonian Center for Astrophysics USA 108 Stefanie Komossa MPE Germany 109 Vlad Kondratiev ASTRON Netherlands 110 Nick Konidaris Caltech USA 111 Michael Kramer MPI fuer Radioastronomie Germany 112 Shrinivas Kulkarni California Institute of Technology USA 113 Omar Kurtanidze Abastumani Observatory Georgia 114 Don Kurtz University of Central Lancashire UK 115 Stefan Larsson Stockholm University Sweden 116 Joseph Lazio JPL ‐ SPDO USA 117 Matthew Lehner ASIAA China 118 Andrew Levan University of Warwick UK 119 David Levitan Caltech USA 120 Tim Lister Las Cumbres Observatory (LCOGT) USA 121 Kitty Lo University of Sydney Australia 122 Giuseppe Lodato University of Milano Italy 123 Tom Loredo Cornell University USA 124 Jean‐Pierre Macquart ICRAR/Curtin University Australia 125 Greg Madsen The University of Sydney Australia 126 Kate Maguire Oxford UK 127 Ashish Mahabal California Institute of Technology USA 128 Ravinder Manchanda Tata Institute India 129 Ilya Mandel University of Birmingham UK 130 Bruce Margon Univ. California Santa Cruz USA 131 Tom Matheson NOAO USA 132 Jaymie Matthews University of British Columbia Canada 133 Amy McQuillan Oxford University UK 134 John Menzies SAAO South Africa 135 Brian Metzger Princeton University USA 136 Areg Mickaelian Byurakan Astrophysical Observatory (BAO) Armenia 137 Roberto Mignani MSSL‐UCL UK 138 Adam Miller UC Berkeley USA 139 Marc Moniez LAL‐IN2P3‐CNRS France 140 Paul Moran Centre for Astronomy NUI Galway Ireland 141 Takashi Moriya IPMU, University of Tokyo Japan 142 Tomoki Morokuma University of Tokyo Japan 143 Nami Mowlavi University of Geneva Switzerland 144 Carole Mundell ARI, Liverpool JM Uni UK 145 Tara Murphy University of Sydney Australia 146 Samaya Nissanke Caltech USA 147 Andrew Norton The Open University UK 148 Peter Nugent LBNL/UCB USA 149 Laura Nuttall Cardiff University UK 150 Kieran O'Brien UCSB USA 151 Rachel Osten Space Telescope Science Institute USA 152 Liudmilla Pakuliak MAO NASU Ukraine 153 Yen‐Chen Pan University of Oxford UK 154 Javier Pascual Instituto de Astrofísica de Andalucía‐CSIC Spain 155 Joe Patterson Columbia Univ. USA 156 Nikki Pekeur Durham University UK 157 Karim Pichara Harvard USA 158 Tsvi Piran The Hebrew University Israel 159 Peter Plavchan Caltech/NExScI USA 160 Joël Poels Institute Astrophysics and Geophysics, University of Liège Belgium 161 Steve Potter South African Astronomical Observatory South Africa 162 Valeriu Predoi Cardiff University UK 163 Larry Price Caltech USA 164 Francesca Primas ESO Germany 165 Tom Prince Caltech USA 166 Chris Pritchet University of Victoria Canada 167 Pavlos Protopapas Harvard‐Smithsonian Center for Astrophysics USA 168 Gavin Ramsay Armagh Observatory UK 169 Colorado Reed University of Iowa USA 170 Armin Rest STScI USA 171 Joey Richards UC Berkeley USA 172 Barney Rickett University of California San Diego USA 173 Stephen Ridgway NOAO USA 174 Lorenzo Rimoldini University of Geneva Switzerland 175 Pete Roming Southwest Research Institute USA 176 Elena M. Rossi Leiden Observatory Netherlands 177 Arnold Rots CfA/SAO USA 178 Slavek Rucinski University of Toronto Canada 179 Bob Rutledge McGill University Canada 180 David Schade National Research Council Canada Canada 181 Bart Scheers API/CWI Netherlands 182 Pim Schellart Radboud University Nijmegen Netherlands 183 Brian Schmidt The Australian National University Australia 184 Linda Schmidtobreick ESO Germany 185 Jeremy Schnittman NASA Goddard USA 186 Josiah Schwab UC Berkeley USA 187 Alex Schwarzenberg‐CzernyCopernicus Astronomical Centre & Poznań University Poland 188 Vicky Scowcroft Carnegie Observatories USA 189 Rob Seaman NOAO USA 190 Alberto Sesana Albert Einstein Institute Germany 191 Vycheslav Shalyapin Institute for Radiophysics and Electronics Ukraine 192 Hiromoto Shibahashi University of Tokyo Japan 193 I Chun Shih Institute of Astronomy, National Tsing Hua University China 194 Min‐Su Shin University of Michigan USA 195 Andrew Siemion University of California, Berkeley USA 196 Leo Singer California Institute of Technology USA 197 Greg Sivakoff University of Alberta Canada 198 Stephen Smartt Queen's University Belfast UK 199 Arfon Smith University of Oxford / Galaxy Zoo UK 200 Ben Stappers University of Manchester UK 201 Rhaana Starling University of Leicester UK 202 Danny Steeghs University of Warwick UK 203 Iain Steele Liverpool JMU UK 204 Rachel Street LCOGT USA 205 Mark Sullivan University of Oxford UK 206 László Szabados Konkoly Observatory Hungary 207 Sumin Tang Harvard University USA 208 Sander ter Veen Radboud University Nijmegen Netherlands 209 Victor Terron Institute of Astrophysics of Andalusia, IAA‐CSIC Spain 210 Nozomu Tominaga Konan University/IPMU Japan 211 Eleonora Troja NASA/GSFC USA 212 Cathryn Trott ICRAR/Curtin University Australia 213 David Tsang California Institute of Technology USA 214 Milcho Tsvetkov Institute of Astronomy, BAS Bulgaria 215 Katya Tsvetkova Institute of Astronomy, BAS Bulgaria 216 Rachel Tunnicliffe University of Warwick UK 217 David Turner Saint Mary's University Canada 218 Joeri van Leeuwen ASTRON Netherlands 219 Sjoert van Velzen Radboud University Nijmegen Netherlands 220 Tom Vestrand Los Alamos National Laboratory USA 221 Norman Walker The Stargazers Trust USA 222 Mark Walker Manly Astrophysics Australia 223 Lucianne Walkowicz Princeton University USA 224 Patrick Wallace STFC / RAL Space UK 225 Brian Warner University of Cape Town South Africa 226 Randall Wayth Curtin University Australia 227 Barry Welsh SSL/UC Berkeley USA 228 Nicholas White NASA Goddard Space Flight Center USA 229 Patricia Whitelock SAAO and University of Cape Town South Africa 230 Peter Williams UC Berkeley USA 231 Roy Williams Caltech/LIGO USA 232 Patrick Woudt University of Cape Town South Africa 233 K.T. Wraight Open University UK 234 Lukasz Wyrzykowski Institute of Astronomy University of Cambridge UK 235 Rosie Wyse Johns Hopkins University USA 236 Ofer Yaron Weizmann Institute Israel 237 Kimon Zagkouris Oxford University UK 238 Ashley Zauderer Harvard USA 239 Chris Wolf Oxford University UK

IAU Symposium 286 – Post meeting report

1.- Meeting number 286

2.- Title of the meeting Comparative Magnetic Minima: Characterizing Quiet Times in the Sun and Stars

3.- Coordinating Division Division II

4.- Dedicated to

5.– Location Auditorio Adolfo Calle, Primitivo de la Reta 1050, Ciudad de Mendoza, Mendoza, Argentina

6.- Dates of meeting 2 – 7 October, 2011

7.- Number of participants 93 persons of which 26 received support from IAU as indicated in the attachment.

8.- Countries represented 23 countries as follows: Argentina, Belgium, Brazil, Colombia, Costa Rica, Denmark, Finland, France, Germany, Hungary, India, Israel, Italy, Japan, Mexico, Peru, Romania, Russia, Turkey, Spain, Sweden, Switzerland, U.K., U.S.A.

9.- Report submitted by Cristina H. Mandrini, Instituto de Astronomía y Física del Espacio, IAFE, UBA-CONICET

10.- Date and place 14 November, 2011, Ciudad de Buenos Aires, Argentina

11.- Signature of SOC Chairpersons

Dr. Hebe Cremades – SOC Co-chair Dr. Sarah Gibson – SOC Co-chair

IAU Symposium 286 – Attached information

Summary of scientific program Keynote talks: 1 Invited talks: 28 Solicited talks: 6 Contributed talks: 28 Closing discussion: 1 Poster presentations: 31

A public outreach talk was given at the end of the symposium in Spanish. Amateur astronomers, high school teachers and students, and the general public were invited to attend.

Final detailed program

Monday 3 October

8:30 – 9:20 Registration 9:20 – 9:40 Welcome Words

Session 1 – Solar and Stellar Minima (Chairs: Hebe Cremades, Sarah Gibson)

9:40 – 10:25 Keynote Talk - The Nature and Significance of Solar Minima Eric Priest 10:25 – 10:55 Invited Talk - Solar and Stellar Activity Diagnostics and Indices Michael Thompson

10:55 – 11: 25 Coffee break

11:25 – 11:45 Solicited Talk - How Well Do We Know Sunspot Number? Leif Svalgaard

Session 2 – Dynamos and Cycle Variability (Chairs: Daniel Gómez, Gustavo Guerrero)

11:45 – 12:15 Invited Talk - Dynamo Action and Magnetic Activity in the Sun and Stars A. Sacha Brun 12:15 – 12:45 Invited Talk - Cycles and Cycle Modulation in Large-Scale Turbulent Dynamos Axel Brandenburg 12:45 – 13:00 Contributed Talk - Magnetic Helicity Fluxes and their Effect on the Simon Candelaresi, A. Brandenburg

13:00 - 15:00 Lunch break

15:00 – 15:30 Invited Talk - Kinematic Dynamo Models of the : Past, Present, and Future Dibyendu Nandi 15:30 – 16:00 Invited Talk - Global MHD Simulations of Stellar Dynamos and the Ingredients for Large-scale Field Organization Matthew Browning, B. Brown, M. Miesch, et al. 16:00 – 16:15 Contributed Talk - Dynamo Action and Magnetic Buoyancy in Convection Simulations in Simulated Tachoclines Gustavo Guerrero, P. Käpylä 16:15 – 16:30 Contributed Talk – Tayler Instability and Stellar Magnetic Fields Fabio del Sordo, A. Brandenburg 16:30 – 16:45 Contributed Talk - Understanding the Origin of the Extended Minimum of Sunspot Cycle 23 Andrés Muñoz-Jaramillo, D. Nandy, P.C.H. Martens

16:45 – 17: 15 Coffee break

17:15 – 19:00 Poster Session

Tuesday 4 October

8:15 – 9:15 Registration

Session 2 – Dynamos and Cycle Variability (Chairs: Daniel Gómez, Gustavo Guerrero)

9:15 – 9:45 Invited Talk - Helioseismic Probing of Dynamo Related Flows Michael Thompson (on behalf of Frank Hill) 9:45 – 10:00 Contributed Talk - Analyzing the Evolution of the Photospheric Magnetic Field in Terms of Spherical Harmonics and Consequences for the Solar Dynamo Marc DeRosa, A.S. Brun, J.T. Hoeksema

Session 3 – Comparative Solar Minima from Sun to Earth (Chairs: Margit Haberreiter, Andrey Tlatov, David Webb)

10:00 – 10:30 Invited Talk – : A View of the Solar Interior Yvonne Elsworth 10:30 – 10:45 Contributed Talk - Reconstruction of Magnetic Field Surges to the Poles from Sunspot Impulses Nadezhda Zolotova, D.I. Ponyavin

10:45 – 11:15 Coffee break

11:15 – 11:45 Invited Talk - Total Solar Irradiance, Absolute Value and an Estimate of a Long-term Trend from Minimum to Minimum Werner Schmutz, A. Fehlman, W. Finsterle, M. Suter 11:45 – 12:00 Contributed Talk - The Ni I Lines in the Solar Spectrum Mariela Vieytes, P. Mauas, J. Fontenla 12:00 – 12:15 Contributed Talk - Modeling the Solar EUV Variability Margit Haberreiter 12:15 – 12:30 Contributed Talk - The Use of 17 GHz Radio Emission to Characterize the Solar Minimum Caius Selhorst, L. Svalgaard, C.G. Giménez de Castro, et al. 12:30 – 13:00 Invited Talk - Polar Magnetic Fields and Coronal Holes during the Recent Solar Minima Giuliana de Toma

13:00 – 15:00 Lunch break

15:00 – 15:30 Invited Talk - Global Magnetic Fields: Variation of Solar Minima Andrey Tlatov, V.N. Obridko 15:30 – 16:00 Invited Talk - The 3D Solar Minimum Corona with Differential Emission Measure Tomography Alberto Vásquez, R.A. Frazin, Z. Huang, et al. 16:00 – 16:15 Contributed Talk - Solar Cycle 23 and 24 Minima Seen through the Eyes of Coronal MHD Models Jon Linker, Z, Mikic, P. Riley, et al. 16:15 – 16:30 Contributed Talk - Large-scale Photospheric Flow Patterns around Coronal Structures Neal Hurlburt 16:30 – 16:45 Contributed Talk - The Role of Streamers in the Deflection of Coronal Mass Ejections: Comparison between STEREO 3D Reconstructions and Numerical Simulations Francesco Zuccarello, A. Bemporad, C. Jacobs, et al.

16:45 – 17:15 Coffee break

17:15 – 17:45 Invited Talk - The Structure of the Heliosphere in Solar Minima and Consequences on Interplanetary Flux Rope Properties Sergio Dasso, A.M. Gulisano, P. Démoulin 17:45 – 18:00 Contributed Talk - Coronal Transients during Two Solar Minima: Their Source Regions and Interplanetary Counterparts Hebe Cremades, C.H. Mandrini, S. Dasso 18:00 – 18:15 Contributed Talk - Dynamo-driven Plasmoid Ejections above a Spherical Surface Jörn Warnecke, A. Brandenburg, D. Mitra 18:15 – 18:30 Contributed Talk - Dynamic Evolution of Interplanetary Wave Shocks Driven by CMEs Pedro Corona Romero, J.A. González Esparza 18:30 – 18:45 Contributed Talk - Dynamical Evolution of Anisotropies of the Solar Wind Magnetic Turbulent Outer Scale María Emilia Ruiz, S. Dasso, W.H. Matthaeus, et al.

Wednesday 5 October

Session 3 – Comparative Solar Minima from Sun to Earth (Chairs: Margit Haberreitter, Andrey Tlatov, David Webb)

9:00 – 9:30 Invited Talk - Interplanetary Conditions: Lessons from this Minimum Janet Luhmann, C.O. Lee, P. Riley, et al. 9:30 – 9:50 Solicited Talk - The Floor in the Solar Wind Magnetic Field: Status Report Ed Cliver 9:50 – 10:05 Contributed Talk – Long-term Solar Wind Variations and the Coming Solar Minimum Ramón López 10:05 – 10:35 Invited Talk – Probing the Heliosphere with the Directional Anisotropy of Galactic Cosmic Ray Intensity Kazuoki Munakata 10:35 – 10:50 Contributed Talk – Search for Solar Energetic Particles Signals on Mexico City Neutron Monitor Database Bernardo Vargas, J.F. Valdés Galicia

10:50 – 11:15 Coffee break

11:15 – 11: 45 Invited Talk – On the Cause of Extremely Low Geomagnetic Activity during the Recent Deep Solar Cycle Minimum Ezequiel Echer, B. Tsurutani, W.D. González 11:45 – 12:00 Contributed Talk – WHI in the Context of a Long and Structured Solar Minimum: An Overview of Sun-to-Earth Observations Sarah Gibson, G. de Toma, Y. Elsworth, et al. 12:00 – 12:30 Invited Talk – Modeling of the Atmospheric Response to a Strong Decrease of the Solar Activity Eugene Rozanov, T. Egorova, A. Shapiro, W. Schmutz 12:30 – 13:00 Invited Talk – Ionosphere and Upper Atmosphere under the Extremely Prolonged Low Solar Activity of Solar Cycle 23 /24 Inez Batista, C.M.N. Candido, C. Brum, M.A. Abdu

13:00 – 15:00 Lunch break

Session 4 – Stellar Cycles (Chairs: Cristina Mandrini, Adriana Válio)

15:00 – 15:30 Invited Talk – Stellar cycles: General Properties and Future Directions Mark Giampapa 15:30 – 16:00 Invited Talk - Investigating Stellar Surface Rotation Using Observations of Starspots Heidi Korhonen 16:00 – 16: 20 Solicited Talk – Modulated Stellar and Solar Cycles: Parallels and Differences K. Oláh, Lidia van Driel- Gesztelyi 16:20 – 16:35 Contributed Talk – The Solar Wind in Time: Internal and External Forcing Jeffrey Linsky, B. Wood, S. Redfield 16:35 – 16:50 Contributed Talk – Stellar Activity Cycles in a Model for Magnetic Flux Generation and Transport Emre Isik

16:50 – 17:15 Coffee break

17:15 – 19:00 Poster Session

Thursday 6 October

Session 4 – Stellar Cycles (Chairs: Cristina Mandrini, Adriana Válio)

9:00 – 9:30 Invited Talk – Magnetic Activity among Cool Stars in the HR-diagram Jürgen Schmitt 9:30 – 9:45 Contributed Talk – On the Origin of Stellar Magnetic Fields Raphael Steinitz, J. Portnoy 9:45 – 10:15 Invited Talk – Semi-empirical Modeling of Solar/Stellar Magnetic Cycles Adriana Válio 10:15 – 10:30 Contributed Talk – The Rotation-activity Connection in Young Low Mass Stars Jenny Rodríguez Gómez, O. Restrepo Gaitán, M. Cuervo Oses, G. Pinzón Estrada 10:30 – 10:50 Solicited Talk – 12 Years of Stellar Activity Observations in Argentina Pablo Mauas, A. Buccino, R. Díaz, et al.

10:50 – 11:15 Coffee break

Session 5 – Grand Minima and Historical Records (Chairs: Alisson Dal Lago, Ilya Usoskin)

11:15 – 11:45 Invited Talk – Stars in Magnetic Grand Minima: Where Are They and What Are They Like? Steven Saar 11:45 – 12:00 Contributed Talk – Soft X-ray Emission as Diagnostics for Maunder Minimum Stars Katja Poppenhäger, J.H.M.M. Schmitt 12:00 – 12:15 Contributed Talk – Is the Small-scale Quiet Sun Dynamo a Pedestal for Solar (and Stellar) Activity? Karel Schrijver 12:15 – 12:35 Solicited Talk – Interplanetary Space Weather and Space Climate Prediction: Opportunities Madhulika Guhathakurta

12:35 – 14:30 Lunch break

14:30 Excursion followed by Conference Dinner

Friday 7 October

Session 5 – Grand Minima and Historical Records (Chairs: Alisson Dal Lago, Ilya Usoskin)

9:00 – 9:30 Invited Talk – Dynamo Models of Grand Minima Arnab R. Choudhuri 9:30 – 9:50 Solicited Talk – A Simple Dynamo Model for Grand Minima and Geomagnetic Reversals Dmitry Sokoloff, G. Sobko, V. Trukhin, V. Zadov 9:50 – 10:05 Contributed Talk – Is Meridional Circulation Important in Modeling the Irregular Solar Cycle? Bidya Karak, A.R. Choudhuri 10:05 – 10:35 Invited Talk – Grand Minima of Solar Activity on Long-term Scales Ilya Usoskin, S.K. Solanki 10:35 – 10:50 Contributed Talk – Geomagnetic Storms and Solar Activity since 1806 Volker Bothmer, E. Bosman

10:50 - 11:15 Coffee break

11:15 – 11:45 Invited Talk – Historical Records of Solar Grand Minima: A Review José Vaquero 11:45 - 12:15 Invited Talk - Does Solar Activity Affect Climate? Blanca Mendoza 12:15 – 12:45 Invited Talk - Effects of Solar Variability on Planetary Plasma Environments and Habitability César Bertucci 12:45 – 13:00 Contributed Talk – EV-Lac as a Potential Host for Habitable Planets Ximena Abrevaya, E. Cortón, P. Mauas

13:00 – 14:30 Lunch break

14:30 – 15:00 Invited Talk - Variations of Solar and Cosmic Ray Cycles at the Maunder Minimum Hiroko Miyahara, Y. Yokoyama, Y.T. Yamaguchi, et al.

Discussion and Summary (Chair: Cristina Mandrini) 15:00 – 16:00 Discussion led by Karel Schrijver Can We Establish if We Are Entering a Grand Minimum, and to Whom would that Matter?

16:00 – 16:15 Publication Plans - Meeting Summary Cristina Mandrini & David Webb – Hebe Cremades & Sarah Gibson

17:30 - 18:30 Public Outreach Talk - Global Warming: Greenhouse Effect or Solar Activity? - Calentamiento Global: ¿Efecto Invernadero o Actividad Solar? Pablo Mauas (the talk will be given in Spanish)

Poster Contributions

S2 – P1 Solar Grand Minima and On-Off Intermittent Dynamo Abraham C.-L. Chian, A. Brandenburg, M.R.E. Proctor, E.L. Rempel S2 – P2 Plasma Flow vs. Magnetic Feature Tracking Speeds in the Sun G. Guerrero, Matthias Rheinhardt, A. Brandenburg, M. Dikpati S2 – P4 Creating a database and Analysis of Sunspots at the Solar Observatory of Ica National University in Peru Lurdes Martínez Meneses, M. Ishitsuka, J. Ishitsuka, H. Trigoso S3 – P5 Study of Ground Cosmic Ray Periodicities during Solar Minimum Using the Multidirectional Muon Detector at the Southern Space Observatory Alisson Dal Lago, L. Ramos Vieira, N.J. Schuch, N.R. Rigozo S3 – P7 Observations of Coronal Holes during Two Solar Minima Heidy Gutiérrez, L. Taliashvili S3 – P8 Coronal Mass Ejection Deflection in the Corona during the Last Two Solar Minima Fernando M. López, H. Cremades, L. Balmaceda S3 – P9 A Cellular Automaton Model for Coronal Heating Marcelo López Fuentes, J.A. Klimchuk S3 – P10 Magneto-seismology of Solar Atmospheric Loops in the Solar Minimum Marialejandra Luna-Cardozo, G. Verth, R. Erdélyi S3 – P11 High Speed Streams in the Solar Wind during the Last Solar Minimum G. Maris, O. Maris, Constantin Oprea, M. Mierla S3 – P12 Geomagnetic Effects on Cosmic Ray Propagation under Different Conditions J.J. Masías Meza, X. Bertou, Sergio Dasso S3 – P13 Forbush Decreases not Related to Transient Solar Events Guadalupe Muñoz Martínez, J.F. Valdés Galicia S3 – P14 The 3D Solar Corona Cycle 24 Rising Phase from SDO/AIA Tomography Federico Nuevo, A.M. Vásquez, R.A. Frazin, Zhenguang Huang, W.B. Manchester S3 – P15 Earth-directed Coronal Mass Ejections and their Geoeffectiveness during the 2007 – 2010 Interval Constantin Oprea, M. Mierla, G. Maris S3 – P16 Evolution of a Very Complex Active Region during the Decay Phase of Cycle 23 Mariano Poisson, M. López Fuentes, C.H. Mandrini, et al. S3 – P17 Cosmic Ray Particles Behavior during the Last Solar Minimum Marlos Rockenbach Da Silva, A. Dal Lago, W.D. González, et al. S3- P18 Radio Signatures Associated with the Origin of LASCO/STEREO CMEs Carolina Salas Matamoros, L. Taliashvili S3- P19 Very Intense Geomagnetic Storms: Solar Sources, Characteristics and Cycle Distribution Natalia Szajko, G. Cristiani, C.H. Mandrini, A. Dal Lago S3 – P20 A Solar Station in Ica: A Research Center to Improve Education at the University and Schools Raul Terrazas Ramos, M. Ishitsuka, J. Ishitsuka, H. Trigoso S4 – P21 Solar Radius and Limb Brightening Variability in the Submillimetric Range Laura A. Balmaceda, A. Válio, C.L. Selhorst S4 – P22 A Statistical Analysis of the H – Ca II K Relation for Solar Type Stars of Different Activity Levels A.P. Buccino, Mariela C. Vieytes, P.J.D. Mauas S4 – P23 Determination of the Effective Temperature from H Spectral Line Analysis of Solar Type Stars Deysi Cornejo Espinoza, I. Ramírez, P. Barklem, W. Guevara Day S4 – P24 Calibrating the Sun-as-a-star: Using Hinode XRT to Measure Stellar Coronae Steven H. Saar, P. Testa S5 – P25 Potential Energy Stored by Planets and Grand Minima Events Rodolfo Cionco S5 – P26 A new Imminent Grand Minima? Rodolfo Cionco, R.H. Compagnucci S5 – P27 Long-term Relation between Sunspot Activity and Surface Temperature at Different Geographical Regions M.P. Souza Echer, Ezequiel Echer, W.D. González, et al. S5 – P28 Parallels among the “Music Scores” of Solar Cycles, Space Weather and Earth’s Climate Z. Kolláth, K. Oláh, Lidia van Driel-Gesztelyi S5 – P29 TTVs Detection in Southern Hemisphere Stars Romina , A.P. Buccino, E. Jofré, et al. S5 – P30 Climate Interaction Mechanism between Solar Activity and Terrestrial Biota Jaime Osorio Rosales, B. Mendoza Ortega S5 – P31 The Coronae of Ca II HK-selected Magnetic Grand Minima Candidate Stars Steven H. Saar, P. Testa Late Posters S3 – P32 Seeing Measurement at Sasahuine Mountain, Moquegua, Peru M. Huamán, W. Guevara Day, E. Meza, J. Samanes, P. Becerra, Cristian Ferradas S3 – P33 Installation and Operation of the Water Cherenkov Detector for the Large Aperture GRB Observatory (LAGO) L.J. Otiniano Ormachea, Edith Tueros Cuadros, W. Guevara Day (LAGO collaboration)

Scientific Organizing Committee

Hebe Cremades (Argentina, Co-chair) Sarah Gibson (USA, Co-chair) Tom Ayres (USA) Alisson Dal Lago (Brazil) Daniel Gomez (Argentina) Manuel Guedel (Austria) Gustavo Guerrero (Sweden) Jeffrey Hall (USA) Margit Haberreiter (Switzerland) Joanna Haigh (UK) Kanya Kusano (Japan) Cristina Mandrini (Argentina) Georgeta Maris (Romania) Valentin Martinez Pillet (Spain) Andrey Tlatov (Russia) Ilya Usoskin (Finland) Adriana Valio (Brazil)

Local Organizing Committee

Cristina Mandrini (IAFE, UBA-CONICET, Buenos Aires, Argentina, Chair) Laura Balmaceda (ICATE and UNSJ, San Juan, Argentina ) Hebe Cremades (UTN and CONICET, Mendoza, Argentina) German Cristiani (IAFE, UBA-CONICET, Buenos Aires, Argentina) Sergio Dasso (IAFE, UBA-CONICET, and Dept. of Physics, FCEN, Buenos Aires, Argentina) Marcelo Lopez Fuentes (IAFE, UBA-CONICET, Buenos Aires, Argentina) Maria Luisa Luoni (IAFE, UBA-CONICET, Buenos Aires, Argentina)

List of participants

AB C DE 1 Order Name Affiliation Country Gender Ximena Abrevaya Instituto de Astronomía y Física Argentina 2 1 del Espacio – IAFE F Laura Balmaceda Instituto de Ciencias Astronómicas, Argentina 3 2 de la Tierra y del Espacio - ICATE F Inez Batista Instituto Nacional de Pesquisas Brazil 4 3 Espaciais – INPE F César Bertucci Instituto de Astronomía y Física Argentina 5 4 del Espacio – IAFE M Volker Bothmer Institute for Astrophysics Germany 6 5 University of Göttingen M Axel Brandenburg Nordic Institute for Theoretical Sweden 7 6 Physics - Nordita M 8 7 Matthew Browning CITA - University of Exeter U.K. M 9 8 Allan Sacha Brun CEA – Saclay France M Simon Candelaresi Nordic Institute for Theoretical Sweden 10 9 Physics - Nordita M 11 10 Abraham Chian Paris Observatory - Meudon France M 12 11 Arnab Choudhuri Indian Institute of Science India M Rodolfo G. Cionco Universidad Tecnológica Nacional Argentina 13 12 Fac. Regional San Nicolás M 14 13 Edward Cliver Air Force Research Laboratory U.S.A. M Deysi V. Cornejo Espinoza Comisio n Nacional de Investigacio n Perú 15 14 y Desarrollo Aeroespacial – CONIDA F 16 15 Pedro Corona Romero Instituto de Geofísica – UNAM México M Hebe Cremades Universidad Tecnológica Nacional Argentina 17 16 Fac. Regional Mendoza F Maximiliano Crescitelli Universidad Tecnológica Nacional Argentina 18 17 Fac. Regional Mendoza M Germa n Cristiani Instituto de Astronomía y Argentina 19 18 Física del Espacio - IAFE M Alisson Dal Lago Instituto Nacional de Pesquisas Brazil 20 19 Espaciais – INPE M Sergio Dasso Instituto de Astronomía y Argentina 21 20 Física del Espacio - IAFE M Giuliana de Toma High Altitude Observatory – National U.S.A. 22 21 Center for Atmospheric Research F Fabio del Sordo Nordic Institute for Theoretical Sweden 23 22 Physics - Nordita M Marc DeRosa Lockheed Martin Solar and U.S.A. 24 23 Astrophysics Laboratory M Ezequiel Echer Instituto Nacional de Pesquisas Brazil 25 24 Espaciais – INPE M Yvonne Elsworth School of Physics and Astronomy U.K. 26 25 University of Birmingham F

AB C DE Cristian Ferradas Alva Comisio n Nacional de Investigacio n Perú 27 26 y Desarrollo Aeroespacial – CONIDA M 28 27 Romina García Universidad Nacional de San Juan Argentina F 29 28 Mark Giampapa National Solar Observatory – NOAO U.S.A. M Sarah Gibson High Altitude Observatory – National U.S.A. 30 29 Center for Atmospheric Research F Daniel Go mez Departamento de Física, FCEN Argentina 31 30 Universidad de Buenos Aires M Walter González Instituto Nacional de Pesquisas Brazil 32 31 Espaciais – INPE M Gustavo Guerrero Nordic Institute for Theoretical Sweden 33 32 Physics - Nordita M Madhulika Guhathakurta Heliophysics Division U.S.A. 34 33 NASA Headquarters F Heidy Gutie rrez Centro de Investigaciones Espaciales Costa Rica 35 34 Universidad de Costa Rica F Margit Haberreiter Physikalisch-Meteorologisches Switzerland 36 35 Observatorium Davos – WRC F Neal Hurlburt Lockheed Martin Advanced U.S.A. 37 36 Technology Center M Francisco Iglesias Universidad Tecnológica Nacional Argentina 38 37 Fac. Regional Mendoza M 39 38 Emre Isik Istanbul Kultur University Turkey M 40 39 Bidya B. Karak Indian Institute of Science India M Heidi Korhonen Niels Bohr Institute Denmark 41 40 University of Copenhagen F 42 41 Jon Linker Predictive Science Inc. U.S.A. M Jeffrey Linsky Joint Institute for Laboratory U.S.A. 43 42 Astrophysics - University of Colorado M Ramón López Department of Physics U.S.A. 44 43 University of Texas at Arlington M 45 44 Fernando López Universidad Nacional de San Juan Argentina M Marcelo López Fuentes Instituto de Astronomía y Argentina 46 45 Física del Espacio - IAFE M Janet Luhmann Space Sciences Laboratory U.S.A. 47 46 University of California, Berkeley F Marialejandra Luna Cardozo Instituto de Astronomía y Física Argentina 48 47 del Espacio – IAFE F María Luisa Luoni Instituto de Astronomía y Argentina 49 48 Física del Espacio - IAFE F Cristina H. Mandrini Instituto de Astronomía y Argentina 50 49 Física del Espacio - IAFE F Lurdes Martínez Meneses Universidad Nacional Perú 51 50 San Luis Gonzaga de Ica F Pablo Mauas Instituto de Astronomía y Física Argentina 52 51 del Espacio – IAFE M 53 52 Blanca Mendoza Ortega Instituto de Geofísica – UNAM México F 54 53 Hiroko Miyahara The University of Tokyo Japan F Kazuoki Munakata Physics Department Japan 55 54 Shinshu University M Andrés Mun oz Jaramillo Harvard-Smithsonian Center U.S.A. 56 55 for Astrophysics M

AB C DE Dibyendu Nandi Indian Institute of Science, Education India 57 56 and Research, Kolkata M Federico Nuevo Instituto de Astronomía y Física Argentina 58 57 del Espacio – IAFE M Constantin Oprea Institute of Geodynamics Romania 59 58 Romanian Academy M 60 59 Jaime A. Osorio Rosales Instituto de Geofísica – UNAM México M Romina Petrucci Instituto de Astronomía y Física Argentina 61 60 del Espacio – IAFE F Mariano Poisson Instituto de Astronomía y Argentina 62 61 Física del Espacio - IAFE M 63 62 Katja Poppenhaeger Hamburg Observatory Germany F 64 63 Eric Priest St. Andrews University U.K. M Matthias Rheinhardt Nordic Institute for Theoretical 65 64 Physics - Nordita Sweden M Marlos Rockenbach da Silva Universidade do Vale do Paraíba Brazil 66 65 UNIVAP M Jenny M. Rodríguez Gómez Observatorio Astronómico Nacional Colombia 67 66 Universidad Nacional de Colombia F Eugene Rozanov Physikalisch-Meteorologisches Switzerland 68 67 Observatorium Davos – WRC M María Emilia Ruiz Instituto de Astronomía y Argentina 69 68 Física del Espacio - IAFE F 70 69 Steven Saar Smithsonian Astrophysical Observatory U.S.A. M Carolina Salas Matamoros Centro de Investigaciones Espaciales Costa Rica 71 70 Universidad de Costa Rica F 72 71 Jürgen Schmitt Hamburger Sternwarte Germany M Werner Schmutz Physikalisch-Meteorologisches Switzerland 73 72 Observatorium Davos – WRC M Karel Schrijver Lockheed Martin Advanced U.S.A. 74 73 Technology Center M Caius Selhorst Universidade do Vale do Paraíba Brazil 75 74 UNIVAP M 76 75 Dmitry Sokoloff Moscow State University Russia M 77 76 Raphael Steinitz Ben Gurion University Israel M 78 77 Leif Svalgaard Stanford University U.S.A. M Natalia S. Szajko Instituto de Astronomía y Argentina 79 78 Física del Espacio - IAFE F Lela Taliashvili Centro de Investigaciones Espaciales Costa Rica 80 79 Universidad de Costa Rica F Raúl Terrazas Ramos Universidad Nacional Perú 81 80 San Luis Gonzaga de Ica M Michael Thompson High Altitude Observatory – National U.S.A. 82 81 Center for Atmospheric Research M Andrey Tlatov Kislovodsk Mountain Astronomical Russia 83 82 Station – Pulkovo Observatory M Ilya Usoskin Department of Physics Finland 84 83 University of Oulu M 85 84 Adriana Válio CRAAM - Mackenzie University Brazil F 86 85 Lidia van Driel-Gesztelyi Konkoly Observatory Hungary F

AB C DE 87 86 José Vaquero Universidad de Extremadura España M 88 87 Bernardo Vargas Instituto de Geofísica – UNAM México M Alberto Vásquez Instituto de Astronomía y Física Argentina 89 88 del Espacio – IAFE M Mariela C. Vieytes Instituto de Astronomía y Física Argentina 90 89 del Espacio – IAFE F Joern Warnecke Nordic Institute for Theoretical Sweden 91 90 Physics - Nordita M David Webb Institute of Scientific Research U.S.A. 92 91 Boston College M 93 92 Nadezhda Zolotova St. Petersburg State University Russia F Francesco Zuccarello Centrum voor Plasma-Astrofysic Belgium 94 93 KU Leuven M

Scientific summary and highlights of the meeting

IAU Symposium 286, "Comparative Magnetic Minima: Characterizing Quiet Times in the Sun and Stars", was coordinated through Division II, with the strong support of Division IV, including several of their associated commissions. It was held in Mendoza, Argentina from 3 to 7 October 2011. The symposium attracted scientific experts on the various topics pertinent to the meeting from all over the world. The goal of IAU Symposium 286 was to consider solar and stellar minima, from generative dynamo mechanisms to in- depth analyses from Sun to Earth for recent well-observed and modeled minima, to a range of stellar cyclic activity, to outlier "grand minima". Solar, heliospheric, geospace, atmospheric, stellar, and planetary sciences were included in the meeting's scope.

Solar and stellar minima represent times of low magnetic activity and simple helio/asterospheres. They are, thus, excellent targets for interdisciplinary, system-wide studies of the origins of stellar variability and consequent impacts on planetary systems. The recent solar minimum extended longer and was "quieter" than any we have observed in the Space Age, inspiring both scientific and public interest. A rich variety of satellite and ground- based observations, in conjunction with theoretical and numerical modeling advances, have allowed us to probe the peculiarities of this minimum as never before. The implications are far-reaching, connecting Earth to Sun to stars, radio to X-ray to cosmic rays, and the plethora of observations of recent minima to the Sun's past behavior as preserved in cosmogenic isotopes and historical sunspot and auroral records.

At the meeting, both invited and contributed presentations were given describing how magnetic fields can be cyclically generated in solar and stellar interiors via various dynamo processes. Numerical models have increased in complexity to the point where many observed aspects of the cycles in the Sun and stars are captured, although mysteries remain such as the origins of extended, or "Grand" Minima. Both stellar observations and historical and cosmogenic records at the Earth were presented to form a basis of understanding of such fascinating intervals, and of solar/stellar long-term variability in general. Along the same lines, a simple method to reconcile the Zürich Sunspot Number and the Group Sunspot Number was presented, with important and wide ranging implications towards an agreed upon and vetted single sunspot series for use in the future.

Detailed examination of the recent extended solar minimum revealed that it was the lowest and longest minimum in about a century, having weak polar magnetic fields, a complex corona and heliosphere, and recurrent high-speed streams. Simultaneously, it was found that solar minima do not all look alike, given that the Sun can have different magnetic flux configurations even during very quiet times, yielding distinct 3D magnetic flux distributions and, therefore, diverse structure of the corona and heliosphere. The larger fraction of higher-order harmonic content implicates that the corona is generally far from dipolar, so that the solar wind has many low- to mid-latitude coronal-hole sources. The many boundaries of these sources, including pseudo-streamers (large-scale closed fields that do not overlie the main solar neutral line), contribute with many transients to the solar wind, seen as blobs and other non-explosive features in images and as features with ICME-like characteristics at 1 AU. During this recent minimum, the solar field has achieved a solar maximum-like corona and solar wind source situation but with weak magnetic fields and associated weak heating. The discussed results point out the need for textbooks and educators to revise the way they describe the solar wind and its sources.

In addition, the recent extended solar minimum provoked discussions on the possibility of a trend in the Sun's current magnetic cycles towards a Grand Minimum, and the potential implications for the Earth's climate. For instance, there is evidence that a strong decrease of the solar activity can lead to a delay of ozone recovery, partially compensating greenhouse warming, and that irradiance variability is the most important forcing for global problems. A combination of the bottom-up and top-down models seems appropriate for the radiative solar forcing of the atmosphere. The phase shift between the solar radiative forcing of surface climate and the solar cycle, indicated by SORCE measurements, will have an important effect on climate modeling. Although the forcing due to anthropogenic influences is about seven times larger than the radiative solar forcing, it can be assured that solar activity does affect climate, establishing the need for a constrained set of future solar forcings and maintenance, and extension, of all relevant observations.

The question of the origins and implications of cyclic behavior, for the Sun-Earth system and also for other stellar-planetary systems, was the subject of several presentations. For instance, it was shown that induced magnetospheres, such as that of Venus, directly interact with the solar wind and, therefore, are more prone to atmospheric evolution than intrinsic magnetospheres. Venus plasma regions and escape rates seem to be strongly influenced by the solar cycle and by the solar wind pressure. On the other hand, Mars boundaries do not appear to be so dependent on the solar cycle phase, though simulations suggest that the escape rate is. Current estimations of the escape rates are of the order of 1025 particles per second, but these estimates may double and even increase by an order of magnitude during stormy space weather. The role of the exosphere in the interaction needs to be further assessed.

This symposium was undoubtedly unique in the sense that it brought a diverse group of scientists that were able to take part in discussions, appreciate the scientific disciplines of others, and discover the common aspects of the physical processes involved in the different studied environments from Sun to Eath, and stars to planets.

The Symposium SOC was chaired by Sarah Gibson and Hebe Cremades, the LOC by Cristina Mandrini, and the editors of the Proceedings are Cristina Mandrini and David Webb.